ESASky TAP
ESASky
ivo://esavo/esasky/tap
European Space Agency
Bruno Merin
esdc_leads@cosmos.esa.int
+34918131456
ESA, ESASky, Archive, ESAC
ESASky is a science-driven discovery portal providing full access to the entire sky as observed with all ESA Space astronomy missions. This service provides access to catalogues, observations, and spectra hosted at the ESAC Science Data Centre.
https://sky.esa.int
https://sky.esa.int/esasky-tap/tap
ADQL
2.0
2.1
ADQL 2.1
Returns a text representation of array dimensions
Parameters:
n: Input array.
Returns the requested element (second argument) of the provided array as first argument in the input
Parameters:
n: Input array.
position: array position of the element to be retrieved where position = 1 refers to the first array element
Returns the length of the requested array dimension
Parameters:
n: Input array.
dim: Input dimension.
Returns the number of dimensions of the array.
Parameters:
n: Input array.
Returns the astrometric parameter errors double array to be used as input for epoch_prop() function
Parameters:
e_ra_deg: Standard Error in Right Ascension (mas)
e_de_deg: Standard Error in Declination (mas)
e_plx: Standard Error in Parallax (mas)
e_pm_ra: Standard Error in Proper Motion in RA (mas/yr)
e_pm_de: Standard Error in Proper Motion in Dec (mas/yr)
de_ra: Correlation Coefficient RA/Dec
plx_ra: Correlation Coefficient Parallax/RA
pm_ra_ra: Correlation Coefficient Proper Motion in RA/RA
pm_de_ra: Correlation Coefficient Proper Motion in Dec/RA
plx_de: Correlation Coefficient Parallax/Dec
pm_ra_de: Correlation Coefficient Proper Motion in RA/Dec
pm_de_de: Correlation Coefficient, Proper Motion in Dec/Dec
pm_ra_plx: Correlation Coefficient Proper Motion in RA/Parallax
pm_de_plx: Correlation Coefficient, Proper Motion in Dec/Parallax
pm_de_pm_ra: Correlation Coefficient, Proper Motion in RA/Proper Motion in Dec
parallax: Parallax (mas)
radial_velocity: Radial Velocity (km/s)
e_rv: Standard Error in Radial Velocity (km/s)
Returns the astrometric parameters double array to be used as input for epoch_prop() function
Parameters:
ra: Right Ascension (deg)
de: Declination (deg)
parallax: Parallax (mas)
pm_ra: Proper Motion in Right Ascension (mas/yr)
pm_de: Proper Motion in Declination (mas/yr)
radial_velocity: Radial Velocity (km/s)
Returns the total number of elements in the array, or 0 if the array is empty.
Parameters:
n: Input array.
For an array of input conditions and results, return the first one found true.
Parameters:
default_value: Value to return if all conditions are false.
conditions: Input conditions array.
results: Input results array.
For an array of input conditions and results, return the first one found equal to input value.
Parameters:
input_value: Value to compare condition values with.
default_value: Value to return if none of condition_values equal input_value.
condition_values: Input results array.
results: Input results array.
For input tables, create a positional crossmatch for input radius and store it in a separate table.
Parameters:
table_schema_a: First table schema.
table_name_a: First table name.
table_schema_b: Second table schema.
table_name_b: Second table name.
radius: Crossmatch radius.
output_table_name: Output table name.
Returns a DATE value that represents the current date
Parameters:
Returns all six input parameters (ra,dec,parallax,pm_ra,pm_dec,radial_velocity) propagated at the new arbitrary input epoch. Please note that the input argument radial_velocity denotes radial velocity in km/s while the corresponding output quantity is the radial proper motion in mas/yr computed as radial_velocity * parallax / 4.740,470,464
Parameters:
ra: Right Ascension (deg)
de: Declination (deg)
parallax: Parallax (mas)
pm_ra: Proper Motion in Right Ascension (mas/yr)
pm_de: Proper Motion in Declination (mas/yr)
radial_velocity: Radial Velocity (km/s)
ref_epoch: Reference Julian Epoch
out_epoch: Final Julian Epoch
Returns all six input parameters (ra,dec,parallax,pm_ra,pm_dec,radial_velocity) propagated at the new arbitrary input epoch. Please note that the input argument radial_velocity denotes radial velocity in km/s while the corresponding output quantity is the radial proper motion in mas/yr computed as radial_velocity * parallax / 4.740,470,464
Parameters:
astrometric_parameters: Array with the full six input parameters needed (ra[deg],dec[deg],plx[mas],pm_ra[mas/yr],pm_dec[mas/yr],pm_rv[mas/yr])
ref_epoch: Reference Julian Epoch
out_epoch: Final Julian Epoch
Returns the propagated covariance matrix from the epoch_prop function
Parameters:
ra: Right Ascension (deg)
dec: Declination (deg)
parallax: Parallax (mas)
pm_ra: Proper Motion in Right Ascension (mas/yr)
pm_de: Proper Motion in Declination (mas/yr)
radial_velocity: Radial Velocity (km/s)
e_ra_deg: Standard Error in Right Ascension (mas)
e_de_deg: Standard Error in Declination (mas)
e_plx: Standard Error in Parallax (mas)
e_pm_ra: Standard Error in Proper Motion in RA (mas/yr)
e_pm_de: Standard Error in Proper Motion in Dec (mas/yr)
e_rv: Standard Error in Radial Velocity (km/s)
de_ra: Correlation Coefficient RA/Dec
plx_ra: Correlation Coefficient Parallax/RA
plx_de: Correlation Coefficient Parallax/Dec
pm_ra_ra: Correlation Coefficient Proper Motion in RA/RA
pm_ra_de: Correlation Coefficient Proper Motion in RA/Dec
pm_ra_plx: Correlation Coefficient Proper Motion in RA/Parallax
pm_de_ra: Correlation Coefficient Proper Motion in Dec/RA
pm_de_de: Correlation Coefficient, Proper Motion in Dec/Dec
pm_de_plx: Correlation Coefficient, Proper Motion in Dec/Parallax
pm_de_pm_ra: Correlation Coefficient, Proper Motion in RA/Proper Motion in Dec
ref_epoch: Reference Julian Epoch (yr)
out_epoch: Final Julian Epoch (yr)
Returns the error vector with the uncertainties associated to the propagated astrometric parameters plus the set of propagated correlation parameters
Parameters:
astrometric_parameters: Array with the full six input parameters needed (ra[deg],dec[deg],plx[mas],pm_ra[mas/yr],pm_dec[mas/yr],pm_rv[mas/yr])
astrometric_parameter_error: Array with the 21 covariance matrix elements (output from astrometric_parameter_error ADQL function)
ref_epoch: Reference Julian Epoch
out_epoch: Final Julian Epoch
Returns the error vector with the uncertainties associated to the propagated astrometric parameters plus the set of propagated correlation parameters
Parameters:
ra: Right Ascension (deg)
de: Declination (deg)
parallax: Parallax (mas)
pm_ra: Proper Motion in Right Ascension (mas/yr)
pm_de: Proper Motion in Declination (mas/yr)
radial_velocity: Radial Velocity (km/s)
e_ra_deg: Standard Error in Right Ascension (mas)
e_de_deg: Standard Error in Declination (mas)
e_plx: Standard Error in Parallax (mas)
e_pm_ra: Standard Error in Proper Motion in RA (mas/yr)
e_pm_de: Standard Error in Proper Motion in Dec (mas/yr)
e_rv: Standard Error in Radial Velocity (km/s)
de_ra: Correlation Coefficient RA/Dec
plx_ra: Correlation Coefficient Parallax/RA
pm_ra_ra: Correlation Coefficient Proper Motion in RA/RA
pm_de_ra: Correlation Coefficient Proper Motion in Dec/RA
plx_de: Correlation Coefficient Parallax/Dec
pm_ra_de: Correlation Coefficient Proper Motion in RA/Dec
pm_de_de: Correlation Coefficient, Proper Motion in Dec/Dec
pm_ra_plx: Correlation Coefficient Proper Motion in RA/Parallax
pm_de_plx: Correlation Coefficient, Proper Motion in Dec/Parallax
pm_de_pm_ra: Correlation Coefficient, Proper Motion in RA/Proper Motion in Dec
ref_epoch: Reference Julian Epoch (yr)
out_epoch: Final Julian Epoch (yr)
Returns the new position (ra,dec) of the source at the new arbitrary input epoch
Parameters:
ra: Right Ascension (deg)
de: Declination (deg)
parallax: Parallax (mas)
pm_ra: Proper Motion in Right Ascension (mas/yr)
pm_de: Proper Motion in Declination (mas/yr)
radial_velocity: Radial Velocity (km/s)
ref_epoch: Reference Julian Epoch
out_epoch: Final Julian Epoch
Select the largest value among given arguments.
Parameters:
v1: First argument.
v2: Second argument.
If input condition is true, return output value. Otherwise return default value.
Parameters:
condition: Value to compare to true.
ouput_value: Value to return if condition is true.
default_value: Value to return if condition is false.
Select the smallest value among given arguments.
Parameters:
v1: First argument.
v2: Second argument.
The function returns the first n characters in the string.
Parameters:
string: a string from which a number of the leftmost characters is returned.
n: an integer that specifies the number of left-most characters in the string should be returned. If n is negative, the function returns the leftmost characters in the string but last |n| (absolute) characters.
The function returns the number of characters in the string.
Parameters:
string: the string that you want to calculate its length.
Returns a null value if value1 equals value2; otherwise it returns value1.
Parameters:
value1: Input value 1.
value2: Input value 2.
The function returns the location of a substring in a string.
Parameters:
substring: the string that you want to locate.
string: the string for which the substring is searched.
Returns the radial velocity in units of mas/yr
Parameters:
pm_rv: Radial proper motion (mas/yr)
parallax: Parallax (mas)
The function returns the last n characters in a string.
Parameters:
string: a string from which a number of the rightmost characters is returned.
n: an integer that specifies the number of right-most characters in the string should be returned. If n is negative, the function returns all characters in the string but first |n| (absolute) characters.
Standard deviation.
Parameters:
n: Input value.
The function returns a part of string.
Parameters:
string: the string that you want to get a part extracted.
start_position: an integer that specifies where you want to extract the substring. If start_position equals zero, the substring starts at the first character of the string. The start_position can be only positive
length: a positive integer that determines the number of characters that you want to extract from the string beginning at start_position. If the sum of start_position and length is greater than the number of characters in the string, the substring function returns the whole string beginning at start_position. The length parameter is optional. If you omit the length parameter, the substring function returns the whole string started at start_position.
Converts input value to BIGINT type.
Parameters:
n: Input value.
Converts input value to BOOLEAN type.
Parameters:
n: Input value.
Converts input value to VARCHAR type.
Parameters:
n: Input value.
Converts input value to DOUBLE type.
Parameters:
n: Input value.
Converts input value to INTEGER type.
Parameters:
n: Input value.
Converts input value to REAL type.
Parameters:
n: Input value.
Converts input value to SMALLINT type.
Parameters:
n: Input value.
The function performs several single-character, one-to-one translation in one operation.
Parameters:
string: the string subjected to translation.
from: a set of characters in the first argument (_string_) that should be replaced.
to: a set of characters that replaces the _from_ in the _string_.
removes the longest string that contains a specific character from a string. By default, the function removes spaces if you don’t specify explicitly which character you want to remove.
Parameters:
characters: optional parameter that defines a literal specifying explicitly which characters you want to remove in the string. Accepted literals are: LEADING, TRAILING and BOTH. Example of use: TRIM(BOTH, string)
string: the string for which the removal is requested. Mandatory parameter: example of use: TRIM(string)
Returns the q3c ipix (Koposov and Bartunov, 2006) for a long/lat pair (it simply wraps the q3c_angpix function).
Parameters:
long: The longitude to compute the ipix for.
lat: The latitude to compute the ipix for.
Returns the new position (ra,dec) of the source at the new arbitrary input epoch
Parameters:
ra: Right Ascension (deg)
de: Declination (deg)
parallax: Parallax (mas)
pm_ra: Proper Motion in Right Ascension (mas/yr)
pm_de: Proper Motion in Declination (mas/yr)
radial_velocity: Radial Velocity (km/s)
ref_epoch: Reference Julian Epoch
out_epoch: Final Julian Epoch
The function transforms ADQL geometries between various reference systems.
Parameters:
from_sys: name of the source reference system.
to_sys: name of the target reference system.
geo: an ADQL geometry (POINT, CIRCLE, POLYGON).
The function returns 1 if, compared case-insensitively, the second argument is in the list of words encoded in the first argument, 0 otherwise.
Parameters:
hashlist: A string containing hash-separated terms.
item: A string containing a single term not containing a hash.
Returns 1 if all tokens from the string needle are contained (in some sense) in the string haystack, 0 otherwise.
Parameters:
needle: A string to locate in haystack.
haystack: A text to match needle in.
This aggregate function returns a histogram of val with nbins+2 elements. Assuming 0-based arrays, results[0] contains the number of underflows (i.e., val < lower), result[nbins+1] the number of overflows. Elements 1…nbins are the counts in nbins bins of width (upper−lower)/nbins. Clients will have to convert back to physical units using some external communication, as there currently is no (meta-) data as lower and upper in the TAP response.
Parameters:
val: the value to bin.
lower: the lower limit of the histogram
upper: the upper limit of the histogram
nbins: the number of "natural" bins in the histogram.
Function returns 1 if the interval [a1…b1] overlaps with the interval [a2…b2].
Parameters:
a1: The lower bound of the first interval.
b1: The upper bound of the first interval.
a2: The lower bound of the second interval.
b2: The upper bound of the second interval.
Evaluates value ILIKE pattern, i.e., pattern is defined as for the SQL LIKE operator, but the match is performed case-insensitively.
Parameters:
value: A string-valued SQL expression.
pattern: A SQL pattern for LIKE evaluation.
Returns a random number drawn from a normal distribution.
Parameters:
mu: The mean of the normal distribution.
sigma: The width of the normal distribution..
Queries Simbad for an identifier and returns the corresponding point.
Parameters:
identifier: A string containing an identifier Simbad can resolve.
An aggregate function returning all values of expression concatenated with delimiter.
Parameters:
expression: A SQL expression giving the strings to concatenate.
delimiter: A string used to concatenate the values of expression in each group.
Converts a timestamp to a Julian date.
Parameters:
d: The SQL timestamp to convert.
Converts a timestamp to modified Julian date.
Parameters:
d: The SQL timestamp to convert.
application/x-votable+xml
votable_gzip
application/x-votable+xml
votable
application/x-votable+xml
votable_plain
text/csv
csv
text/ecsv
ecsv
text/tab-separated-values
tsv
application/json
json
application/fits
fits
text/xml
votable_plain_conesearch
259200
259200
3600
3600
3000000
3000000
100000000
100000000
https://sky.esa.int/esasky-tap/tap/availability
https://sky.esa.int/esasky-tap/tap/tables
https://sky.esa.int/esasky-tap/tap/capabilities
alerts
alerts.mv_v_gravitational_waves_fdw
npix
long
oid
meta.id;meta.main
int
event_page
Web page for evolving status of this GW candidate
meta.ref.url
char
primary
skymap_fits
Sky Map FITS
meta.ref.url;meta.product
char
grace_id
Identifier in GraceDB
meta.id
char
primary
iso_time
Timestamp for detection of this gravitational event
char
primary
alert_type
VOEvent alert type
meta.version
char
far
False alarm rate for GW candidates with this strength or greater
Hz
arith.rate;stat.falsealarm
double
instruments
List of instruments used in analysis to identify this event
meta.code
char
pipeline
Low-latency data analysis pipeline
meta.code
char
bbh
Probability that the source is a binary black hole merger (both objects heavier than 5 solar masses)
stat.probability
double
bns
Probability that the source is a binary neutron star merger (both objects lighter than 3 solar masses)
stat.probability
double
nsbh
Probability that the source is a neutron star-black hole merger (primary heavier than 5 solar masses, secondary lighter than 3 solar masses)
stat.probability
double
mass_gap
Probability that the source has at least one object between 3 and 5 solar masses
stat.probability
double
has_ns
Probability that at least one object in the binary has a mass that is less than 2.83 solar masses
stat.probability
double
has_remnant
Probability that a nonzero mass was ejected outside the central remnant object
stat.probability
double
terrestrial
Probability that the source is terrestrial (i.e., a background noise fluctuation or a glitch)
stat.probability
double
fluence
Estimated fluence of GW burst signal
erg/cm^2
gw.fluence
double
central_freq
Central frequency of GW burst signal
Hz
gw.frequency
double
duration
Measured duration of GW burst signal
s
time.duration
double
gravitational_waves_oid
meta.oid
int
group_id
Data analysis working group
meta.code
char
hardware_inj
Indicates that this event is a hardware injection if 1, no if 0
meta.number
double
internal
Indicates whether this event should be distributed to LSC/Virgo members only
double
open_alert
Indicates that this event is an open alert if 1, no if 0
meta.number
double
packet_type
The Notice Type number is assigned/used within GCN, eg type=152 is an LVC_UPDATE notice
double
pkt_ser_num
A number that increments by 1 each time a new revision is issued for this event
meta.version
double
search
Specific low-latency search
meta.code
char
stcs50
Footprint of 50% probability region
obscore:Char.SpatialAxis.Coverage.Support.Area
char
stcs90
Footprint of 90% probability region
obscore:Char.SpatialAxis.Coverage.Support.Area
char
ra
Right ascension (J2000) of point with highest probability
degrees
pos.eq.ra;meta.main
double
dec
Declination (J2000) of point with highest probability
deg
pos.eq.dec;meta.main
double
alerts.mv_v_icecube_event_fdw
event_page
meta.ref.url
char
primary
notice_type
Notice Type (Gold and Bronze events are single-neutrino events in the IceCube detector with a neutrino energy between sub-PeV to 1 PeV. Gold events are on average ~50% likely to be of astrophysical origin, Bronze events are on average ∼30% likely to be of astrophysical origin. Cascade events are triggers from high energy neutrinos).
char
primary
event_num
Event number
int
primary
run_num
Run number
int
primary
ra
RA location of the event (J2000 epoch)
pos.eq.ra;meta.main
double
dec
Dec location of the event (J2000 epoch)
pos.eq.dec;meta.main
double
energy
For Gold and Bronze events: most probable neutrino energy that would have produced an event with these observed parameters under an astrophysical neutrino signal hypothesis, assuming the best-fit diffuse muon neutrino astrophysical power-law flux ( E^-2.19). For Cascade events: Energy of the neutrino (in TeV).
double
signalness
Probability this is an astrophysical signal relative to backgrounds.
double
stream
Stream number
int
far
False Alarm Rate. For Gold and Bronze events: the rate of background events expected that are 'like this alert' that would be seen by IceCube per year. For Cascade events: specifies how often a trigger of this intensity would happen from just noise fluctuations (an identically 0 value means it was not calculated TBD).
double
discovery_timestamp
Discovery Timestamp
char
primary
dec_1950
Dec location of the event (1950 epoch).
double
dec_current
Dec location of the event (current epoch at time of event)
double
discovery_date
char
discovery_time
char
icecube_event_oid
int
notice_date
Date of the notice
char
npix
Healpix pixel of the center of the observation for nside 256
long
ra_1950
Ra location of the event (1950 epoch)
double
ra_current
Ra location of the event (current epoch at time of event)
double
revision
Revision number
char
src_error
Location uncertainty (radius, statistical plus systematic, 90% containment) in units of degrees
double
src_error50
Location uncertainty (radius, statistical plus systematic, 50% containment) in units of degrees
double
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
title
Title of the notice
char
catalogues
catalogues.integral_ibis
alter_name
Other source identifier
char
e_flux20_40
Uncertainty in flux20_40
mCrab
char
e_flux40_100
Uncertainty in flux40_100
mCrab
char
err_pos
Position error. Expressed as radius of 90% confidence circle.
arcmin
double
flag
Flag on Name. N = A new detection since fourth IBIS/ISGRI catalog (Bird+, 2010).
char
flag1
Low significance warning flag. WARN = the fraction of false sources may be as much as 25%.
char
flag2
Blended source; fluxes may be contaminated.
char
flag3
Source lies in confused region. Around Galactic Center. GCFLAG1 = Source lies within the GC box, and is detected by our standard methods. GCFLAG2 = Clear evidence of emission from the source position in one or more of our maps, but it lies within an unresolved emission region.
char
gallery_url
meta.ref.url
char
primary
pos
char
vari
Variability indicator. Y = bursticity >1.1 (i.e., a 10% increase in significance can be obtained by selecting a single contiguous subset of the data) and a slightly variable source. YY = bursticity of >4 (i.e., a 400% increase in significance), indicating a strongly variable source.
char
name
Primary source identifier
meta.id;meta.main
char
primary
ra
Right ascension of source (J2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination of source (J2000)
deg
pos.eq.dec;meta.main
double
primary
flux20_40
Time-averaged flux in the 20-40 keV band. Appropriate conversion factors are: (20-40keV) 10mCrab=7.57e-11erg/cm2/s=1.71e-3ph/cm2/s.
mCrab
char
primary
flux40_100
Time-averaged flux in the 40-100 keV band. Appropriate conversion factors are: (40-100keV) 10mCrab=9.42e-11erg/cm2/s=9.67e-4ph/cm2/s.
mCrab
char
primary
source_type
Source type classification
char
primary
signif
Maximum significance.
char
primary
exposure
Corrected on-source exposure.
ks
char
primary
catalogues.mv_aspic_fdw
picdr1id
PLATO identifier for asPIC1.1
meta.id;meta.main
int
primary
picdr1
PLATO identifier for asPIC1.1 with version number, PIC DR1 NNNNNNNN
meta.id
char
gaia_dr2
Gaia DR2 sourceId
meta.id
long
ra_deg
Barycentric right ascension of the source in ICRS at Ep=2015.5
deg
pos.eq.ra;meta.main
double
primary
e_ra_deg
Standard error e_RA*=e_RA x cosDE of the right ascension in ICRS at Ep=2015.5
mas
stat.error;pos.eq.ra
double
de_deg
Barycentric declination of the source in ICRS at Ep=2015.5
deg
pos.eq.dec;meta.main
double
primary
e_de_deg
Standard error of the declination in ICRS at Ep=2015.5
mas
stat.error;pos.eq.dec
double
plx
Parallax
mas
pos.parallax.trig
double
primary
e_plx
Standard error on parallax
mas
stat.error;pos.parallax.trig
double
pmra_cosdec
Proper motion in right ascension direction pmRA*=pmRAxcosDE in ICRS at Ep=2015.5
mas/yr
pos.pm;pos.eq.ra
double
primary
e_pmra_cosdec
Standard error on proper motion in right ascension direction
mas/yr
stat.error;pos.pm;pos.eq.ra
double
pmde
Proper motion in declination direction in ICRS at Ep=2015.5
mas/yr
pos.pm;pos.eq.dec
double
primary
e_pmde
Standard error on proper motion in declination direction
mas/yr
stat.error;pos.pm;pos.eq.dec
double
pm
The total proper motion calculated as pm = sqrt(pmRA^2^ + pmDE^2^)
mas/yr
pos.pm;pos.eq
double
primary
e_pm
Error on the total proper motion
mas/yr
stat.error;pos.pm;pos.eq
double
epoch
[2015.5] Reference epoch to which the astrometric source parameters are referred
yr
time.epoch
double
fg
Mean flux in the G band
e-/s
phot.flux;em.opt
double
e_fg
Error on G band mean flux
e-/s
stat.error;phot.flux;em.opt
double
gmag
Mean magnitude in the G band
mag
phot.mag;em.opt
double
primary
e_gmag
Error on mean magnitude in the G band
mag
stat.error;phot.mag;em.opt
double
fbp
Mean flux in the integrated BP band
e-/s
phot.flux;em.opt.B
double
e_fbp
Error on mean flux in the integrated BP band
e-/s
stat.error;phot.flux;em.opt.B
double
bpmag
Mean magnitude in the integrated BP band
mag
phot.mag;em.opt.B
double
primary
e_bpmag
Error in the mean magnitude in the integrated BP band
mag
stat.error;phot.mag;em.opt.B
double
frp
Mean flux in the integrated RP band
e-/s
phot.flux;em.opt.R
double
e_frp
Error on mean flux in the integrated RP band
e-/s
stat.error;phot.flux;em.opt.R
double
rpmag
Mean magnitude in the integrated RP band
mag
phot.mag;em.opt.R
double
primary
e_rpmag
Error in the mean magnitude in the integrated RP band
mag
stat.error;phot.mag;em.opt.R
double
"e(bp/rp)"
BP/RP excess factor
arith.factor;phot.flux;em.opt
double
"bp-rp"
GBP - GRP color
mag
phot.color;em.opt.B;em.opt.R
double
"bp-g"
GBP - G color
mag
phot.color;em.opt.B;em.opt
double
"g-rp"
G - GRP color
mag
phot.color;em.opt;em.opt.R
double
glon
Galactic longitude of the object at Ep=2015.5
deg
pos.galactic.lon
double
primary
glat
Galactic latitude of the object at Ep=2015.5
deg
pos.galactic.lat
double
primary
elon
Ecliptic longitude of the object at Ep=2015.5
deg
pos.ecliptic.lon
double
primary
elat
Ecliptic latitude of the object at Ep=2015.5
deg
pos.ecliptic.lat
double
primary
rest
The estimated distance from Bailer-Jones et al., 2018AJ....156...58B, Cat. I/347
pc
pos.distance
double
primary
rlo
The lower bound of the confidence interval of the estimated distance from Bailer-Jones et al., 2018AJ....156...58B, Cat. I/347
pc
stat.error;stat.min;pos.distance
double
rhi
The higher bound of the confidence interval of the estimated distance from Bailer-Jones et al., 2018AJ....156...58B, Cat. I/347
pc
stat.error;stat.max;pos.distance
double
e_rest
The error in the estimated distance calculated as e_rest = 0.5(rhi - rlo)
pc
stat.error;pos.distance
double
ag
Estimate of the extinction AG in the G band
mag
phys.absorption
double
e_ag
Uncertainty on AG estimate
mag
stat.error
double
"e(bp-rp)"
Estimate of reddening E(GBP-GRP)
mag
phot.color.excess
double
"e_e(bp-rp)"
Uncertainty on reddening E(GBP - GRP)
mag
stat.error
double
"e(b-v)"
Estimate of reddening E(B-V)
mag
phot.color.excess
double
"e_e(b-v)"
Uncertainty on E(B-V) reddening
mag
stat.error
double
extstatus
[0/1] extStatus value. If extStatus=1 the star is outside the limits of the reddening map (from Lallement et al. 2018A&A...616A.132L, see also Appendix E in the paper)
meta.code
int
"(bp-rp)0"
Dereddened (GBP - GRP) color
mag
phot.color
double
"e_(bp-rp)0"
Error on dereddened (GBP - GRP) color
mag
stat.error
double
gaiav0
Dereddened apparent visual magnitude V in the Johnson-Cousin system
mag
phot.mag;em.opt.V
double
primary
e_gaiav0
Error on intrinsic visual magnitude
mag
stat.error
double
bjgaiamv0
Absolute intrinsic visual magnitude obtained as: BJgaiaMV0 = gaiaV0 -5log10rest + 5
mag
phys.magAbs
double
e_bjgaiamv0
Error on absolute intrinsic visual magnitude
mag
stat.error
double
gaiav
Visual apparent magnitude in the Johnson-Cousin system obtained as: gaiaV = gaiaV0 + 3.1E(B-V)
mag
phot.mag;em.opt.V
double
primary
e_gaiav
Error on apparent visual magnitude V
mag
stat.error
double
bjgaiamg0
Absolute intrinsic G magnitude obtained as: BJgaiaMG0 = Gmag -5log10rest +5 -AG
mag
phys.magAbs
double
e_bjgaiamg0
Error on intrinsic absolute G magnitude
mag
stat.error
double
teff
? Estimate of stellar effective temperature
K
phys.temperature.effective
double
e_teff
? Uncertainty on Teff estimate
K
stat.error;phys.temperature.effective
double
rad
? Estimate of stellar radius
Rsun
phys.size.radius
double
e_rad
? Uncertainty on stellar radius estimate
Rsun
stat.error
double
mass
? Estimate of stellar mass
Msun
phys.mass
double
e_mass
? Uncertainty on mass estimate
Msun
stat.error;phys.mass
double
sourceflag
[0/6] Bitmask indicating if the source is a FGK or M star and if the star hosts known planet(s) Bitmask values as follows: 0 = reset all bits; 1 = FGK star; 2 = M star; 4 = Host Planet(s); 5 = FGK star and Host Planet(s); 6 = M star and Host Planet(s)
meta.code
int
contgmag60
? Total G magnitude of the Gaia contaminants within 60 arcsec
mag
phot.mag;em.opt
double
primary
contn60
Total number of Gaia contaminants within 60 arcsec
meta.number
int
contgmag45
? Total G magnitude of the Gaia contaminants within 45 arcsec
mag
phot.mag;em.opt
double
primary
contn45
Total number of Gaia contaminants within 45 arcsec
meta.number
int
contgmag30
? Total G magnitude of the Gaia contaminants within 30 arcsec
mag
phot.mag;em.opt
double
primary
contn30
Total number of Gaia contaminants within 30 arcsec
meta.number
int
catalogues.mv_cat2rxs_fdw
cat2rxs_oid
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
raj2000
Right ascension (J2000) (RA_DEG)
deg
pos.eq.ra;meta.main
double
primary
dej2000
Declination (J2000) (DEC_DEG)
deg
pos.eq.dec;meta.main
double
primary
recno
Record number assigned by the VizieR team. Should Not be used for identification.
meta.record
int
"2rxs"
IAU name (IAU_NAME) (1)
meta.id;meta.main
char
crate
Source count rate (RATE)
ct/s
phot.count;em.X-ray
double
primary
e_crate
Error of the count rate (ERATE)
ct/s
stat.error
double
primary
seq
? Sky field number (SEQ_ID)
meta.id;obs.field
int
exptime
Source exposure time (EXPOSURE)
s
time.duration;obs.exposure
double
primary
inddet
? Source number in a certain sky field (IND_DET)
meta.id;obs.field
short
eximl
Detection likelihood (EXI_ML)
stat.likelihood
double
ext
Source extent in units of image pixels (EXT)
pix
phys.angSize;arith.ratio
double
primary
cts
Background corrected source counts (CTS)
ct
phot.count;em.X-ray
double
extml
Proability of the source extend (EXT_ML)
stat.likelihood
double
primary
e_cts
Error of the source counts (CERR)
ct
stat.error
double
hr1
? Hardness ratio 1 value (HR_1) (2)
phot.flux;arith.ratio
double
primary
hr2
? Hardness ratio 2 value (HR_2) (2)
phot.flux;arith.ratio
double
primary
sflag
? S flag (0=good) (S_flag) (4)
meta.code
short
primary
rahms
Sexadecimal right ascension (J2000) (RA_HMS)
pos.eq.ra
char
dedms
Sexadecimal declination (J2000) (DEC_DMS)
pos.eq.dec
char
glon
Latitude in galactic coordinate (LII)
deg
pos.galactic.lon
double
glat
Longitude in galactic coordinate (BII)
deg
pos.galactic.lat
double
lambda
Latitude in ecliptic coordinate (LAMBDA)
deg
pos.ecliptic.lat
double
beta
Longitude in ecliptic coordinate (BETA)
deg
pos.ecliptic.lon
double
e_ext
Error of the source extent (EXTERR)
pix
stat.error
double
e_hr1
? Error of HR1 (HR_1_err)
stat.error
double
e_hr2
? Error of HR2 (HR_2_err)
stat.error
double
usky
? Unique flag (USKY) (3)
meta.code
short
masked
[1]? Extended emission regions (0=yes 1=no) (Masked)
meta.code
short
fall
[0]? Detection flag of nearby sources (FLAG_all) 0=best
meta.code
short
index
? Running number in catalogue (INDEX)
meta.id
short
ampmax
? Maximum amplitude variability (AMPL_MAX)
src.var.amplitude
double
cm
? Mean count rate value (CM)
ct/s
phot.count;em.X-ray
double
cd
? Standard deviation of CM (CD)
ct/s
stat.error
double
ctslc
? Number of counts calculated from the light curve analysis (CTS_lc)
ct
phot.count
double
c_min
? Minimum count rate ( CMIN)
ct/s
phot.count;em.X-ray
double
c_max
? Maximum count rate ( CMAX)
ct/s
phot.count;em.X-ray
double
e_cmin
? Error of CMIN (EMIN)
ct/s
stat.error
double
e_cmax
? Error of CMAX (EMAX)
ct/s
stat.error
double
chi2lc
? Chi^2^ value from the LC analysis (CHI2_lc)
stat.fit.chi2
double
excvar
? Normalized excess variance (EXCESS_VAR)
stat.variance
double
e_excvar
? One-sigma uncertainty of Exc_Var (UNCERTAINTY)
stat.error
double
sigexc
? Excess variance in units of sigma (Sigma_Excess)
stat.variance
double
nhgal
? Galactic neutral hydrogen density (NH_gal)
10+21cm-2
phys.density;pos.galactic
double
nhfitp
? neutral hydrogen density of PL fits (NH_fit_p)
10+21cm-2
phys.columnDensity
double
e_nhfitp
? Error of NHfitp (NH_err_p)
10+21cm-2
stat.error
double
normp
? Normalization for PL fits (NORM_p)
stat.fit.param
double
e_normp
? Error of NORM_p (NORM_err_p)
stat.error
double
gammap
? Photon index (GAMMA_p)
spect.index
double
e_gammap
? Error of GAMMA_p (GAMMA_err_p)
stat.error
double
ctrspep
? Count rate obtained from the PL fit (CTR_spec_p)
ct/s
phot.count;em.X-ray
double
fluxp
? Absorption corrected flux of PL-fit (FLUX_p)
mW/m2
phot.flux;em.X-ray
double
chi2rspp
? Reduced chi^2 value for the PL-fits (Chi2red_spec_p)
stat.fit.chi2
double
chi2spp
? Chi^2 value for the power-law-fits (Chi2_spec_p)
stat.fit.chi2
double
ndptp
? Number of data points for the PL-fits (Num_Data_pts_p)
meta.number
short
ndfp
? Number of degrees of freedom (PL) (Num_Deg_free_p)
meta.number
short
nhfitm
? Neutral hydrogen density (mekal fits) (NH_fit_m)
10+21cm-2
phys.columnDensity
double
e_nhfitm
? Error of NH_fit_m (NH_err_m)
10+21cm-2
stat.error
double
normm
? Normalization for the mekal fits (NORM_m)
stat.fit.param
double
e_normm
? Error of NORM_m (NORM_err_m)
stat.error
double
tempfitm
? Temperature of the mekal fits (Temp_fit_m)
phys.temperature
double
e_tempfitm
? Error of Temp_fit_m (Temp_err_m)
stat.error
double
ctrspm
? Count rate obtained for the mekal fits (CTR_spec_m)
ct/s
phot.count;em.X-ray
double
fluxm
? Absorption corrected flux (mekal fits) (FLUX_m)
mW/m2
phot.flux;em.X-ray
double
chi2rspm
? Reduced chi^2 value for mekal fits (Chi2red_spec_m)
stat.fit.chi2
double
chi2spm
? Chi^2 value for the mekal fits (Chi2_spec_m)
stat.fit.chi2
double
ndptm
? Number of data points (mekal fits) (Num_Data_pts_m)
meta.number
short
ndfm
? Number of degrees of freedom (mekal) (Num_Deg_free_m)
meta.number
short
nhfitb
? Neutral hydrogen density (bbdy fits) (NH_fit_b)
10+21cm-2
phys.columnDensity
double
e_nhfitb
? Error of NH_fit_b (NH_err_b)
10+21cm-2
stat.error
double
normb
? Normalization for the black body fits (NORM_b)
stat.fit.param
double
e_normb
? Error of the normalization (bbdy fits) (NORM_err_b)
stat.error
double
tempfitb
? Temperature of the black body fits (Temp_fit_b)
phys.temperature
double
e_tempfitb
? Error of Temp_fit_bbdy (Temp_err_b)
stat.error
double
ctrspb
? Count rate for the black body fit (CTR_spec_b)
ct/s
phot.count;em.X-ray
double
fluxb
? Absorption corrected flux (black body) (FLUX_b)
mW/m2
phot.flux;em.X-ray
double
chi2rspb
? Reduced chi^2^ value (black body) (Chi2red_spec_b)
stat.fit.chi2
double
chi2spb
? Chi^2^ value for the black body fits (Chi2_spec_b)
stat.fit.chi2
double
ndptb
? Number of data points (black body) (Num_Data_pts_b)
meta.number
short
ndfb
? Number of degrees of freedom (bbdy) (Num_Deg_free_b)
meta.number
short
xima
X image coordinate (45 arcsec) in image pixel (X_IMA)
pix
pos.cartesian.x;instr.det
double
yima
Y image coordinate (45 arcsec) in image pixel (Y_IMA)
pix
pos.cartesian.y;instr.det
double
e_xima
One-sigma error of X_IMA in image pixel (XERR)
pix
stat.error
double
e_yima
One-sigma error of Y_IMA in image pixel (YERR)
pix
stat.error
double
xsky
X sky coordinates (0.5 arcsec) in sky pixel (X_SKY)
pix
pos.cartesian.x;instr.det
double
ysky
Y sky coordinates (0.5 arcsec) in sky pixel (Y_SKY)
pix
pos.cartesian.y;instr.det
double
curad
[600]? Source extraction radius in sky pixels (CUT_RAD)
pix
phys.angSize
short
fa
Analyzed fraction of cut radius (FA)
stat.fit.param
double
totnum
? Total number of photons read from the PET and analyzed by the maximum likelihood algorithm (TOTNUM)
phot.count;em.X-ray
short
bgr
Background in source extraction region in 1/pix_image (BGR)
pix-1
instr.background
double
vigcor
Vignetting correction factor (VIG_COR)
instr.param
double
rem
[source nrby?] on flags originating from ML-detection (REMARKS)
meta.note
char
sb1
? Counts in band A (SB1)
ct
phot.count;em.X-ray
double
sb2
? Counts in band B (SB2)
ct
phot.count;em.X-ray
double
sb3
? Counts in band C (SB3)
ct
phot.count;em.X-ray
double
sb4
? Counts in band D (SB4)
ct
phot.count;em.X-ray
double
b1
? Background band A with other catalogue entries excised (B1)
ct
instr.background;meta.table
double
b2
? Background band B with other catalogue entries excised (B2)
ct
instr.background;em.opt.B;meta.table
double
b3
? Background band C with other catalogue entries excised (B3)
ct
instr.background;meta.table
double
b4
? Background band D with other catalogue entries excised (B4)
ct
instr.background;meta.table
double
bspa
? Remaining bkg area in square arcmin
arcmin+2
instr.background
double
s1
? Source counts in band A (SB1 - B1*sb_spa/b_spa) (S1)
ct
phot.count;em.X-ray
double
s2
? Source counts in band B (SB2 - B2*sb_spa/b_spa) (S2)
ct
phot.count;em.X-ray
double
s3
? Source counts in band c (SB3 - B3*sb_spa/b_spa) (S3)
ct
phot.count;em.X-ray
double
s4
? Source counts in band D (SB4 - B4*sb_spa/b_spa) (S4)
ct
phot.count;em.X-ray
double
mxmmsl1
? Number of counterparts in the XMM Slew Survey within the distance of 60" (mult_xmmsl1)
meta.number
short
exmmsl1
? Source number of nearest counterpart in the XMM Slew Survey (entr_xmmsl1)
meta.id
int
dxmmsl1
?=0 Distance of nearest XMMSL1 counterpart (dist_xmmsl1)
arcsec
pos.angDistance;src.orbital
double
ra1deg
XMMSL Right ascension (J2000) (RA_xmmsl1)
deg
pos.eq.ra
double
de1deg
XMMSL Declination (J2000) (DEC_xmmsl1)
deg
pos.eq.dec
double
xmmsl1
Source name in the XMM Slew Survey (SRCNAME_xmmsl1)
meta.id
char
crb0
? Broad Band Count rate (RATE_B0_xmmsl1)
ct/s
phot.count;em.X-ray
double
e_crb0
? Broad Band Count rate error (RATE_B0e_xmmsl1)
ct/s
stat.error
double
crb5
? Count rate, energy band 0.5-2keV (RATE_B5_xmmsl1)
c/s
phot.count;em.X-ray
double
e_crb5
? Count rate error, 0.5-2keV (RATE_B5e_xmmsl1)
c/s
stat.error
double
m3xmm
? Number of 3XMM counterparts within the distance of 60"(mult_3xmm)
meta.number
short
e3xmm
? Source number of nearest counterpart in the 3XMM Catalogue (entr_3xmm)
meta.id
int
d3xmm
?=0 Distance of nearest 3XMM counterpart (dist_3xmm)
arcsec
pos.angDistance;src.orbital
double
ra2deg
3XMM Right ascension (J2000) (RA_3xmm)
deg
pos.eq.ra
double
de2deg
3XMM Declination (J2000) (DEC_3xmm)
deg
pos.eq.dec
double
"3xmm"
Source name in the 3XMM Catalogue (SRCNAME_3xmm)
meta.id
char
crep8
? 3XMM Count rate (RATE_EP8_3xmm)
ct/s
phot.count;em.X-ray
double
e_crep8
? 3XMM Count rate error (RATE_EP8e_3xmm)
ct/s
stat.error
double
fluxr
? 3XMM Flux (FLUX_R_3xmm)
mW/m2
phot.flux;em.X-ray
double
e_fluxr
? 3XMM Flux error (FLUX_R_err_3xmm)
mW/m2
stat.error
double
m2rxp
? Number of 2RXP counterparts within the distance of 300" (mult_2rxp)
meta.number
short
e2rxp
? Source number of nearest counterpart in the 2RXP catalogue (entr_2rxp)
meta.id
int
d2rxp
?=0 Distance of 2RXP nearest counterpart (dist_2rxp)
arcsec
pos.angDistance;src.orbital
double
ra3deg
2RXP Right ascension (J2000) (RA_2rxp)
deg
pos.eq.ra
double
de3deg
2RXP Declination (J2000) (DEC_2rxp)
deg
pos.eq.dec
double
"2rxp"
Source name in the 2RXP (SRCNAME_2rxp)
meta.id
char
cr2rxp
? 2RXP Count rate (CRATE_2rxp)
ct/s
phot.count;em.X-ray
double
e_cr2rxp
? 2RXP Count rate error (CRATE_err_2rxp)
ct/s
stat.error
double
etim2rxp
? 2RXP Source exposure time (ExpTime_2rxp) (132)
s
time.duration;obs.exposure
int
obsid
Field number of 2RXP counterpart (ObsID_2rxp) (133)
meta.id;obs
char
m1rxs
? Number of 1RXS counterparts within a distance of 60" (mult_1rxs)
meta.number
short
e1rxs
? Source number of nearest counterpart in the 1RXS catalogue (entr_1rxs)
meta.id
int
d1rxs
?=0 Distance to nearest 1RXS counterpart (dist_1rxs) (136)
arcsec
pos.angDistance;src.orbital
double
ra4deg
1RXS Right ascension (J2000) (RA_1rxs)
deg
pos.eq.ra
double
de4deg
1RXS Declination (J2000) (DEC_1rxs)
deg
pos.eq.dec
double
"1rxs"
Source name in the 1RXS catalogue (SRCNAME_1rxs)
meta.id
char
cr1rxs
? Source count rate in the 1RXS (RATE_1rxs)
ct/s
phot.count;em.X-ray
double
e_cr1rxs
? Error of RATE_1rxs (RATE_err_1rxs)
ct/s
stat.error
double
cts1rxs
? Background corrected src counts 1RXS (CTS_1rxs)
phot.count;em.X-ray
double
e_cts1rxs
? Error of CTS_1rxs (CTS_err_1rxs)
stat.error
double
eximl1rxs
? Background corrected src counts 1RXS (EXI_ML_1rxs)
stat.likelihood
short
expos1rxs
? Source exposure time in 1RXS (EXPOS_1rxs) (145)
s
time.duration;obs.exposure
int
hr11rxs
? 1RXS Hardness ratio 1 value (HR1_1rxs) (5)
phot.flux;arith.ratio
double
e_hr11rxs
? Error of HR1 in the 1RXS (HR1e_1rxs)
stat.error
double
hr21rxs
? 1RXS Hardness ratio 2 value (HR2_1rxs) (5)
phot.flux;arith.ratio
double
e_hr21rxs
? Error of HR2 in the 1RXS (HR2e_1rxs)
stat.error
double
mvv10
? Number of counterparts in the Veron and Verson Catalogue within the distance of 60" (mult_vv10)
meta.number
short
evv10
? Source number of VV10 nearest counterpart (entr_vv10)
meta.id
int
dvv10
?=0 Distance to nearest VV10 counterpart (dist_vv10)
arcsec
pos.angDistance;src.orbital
double
vv10
VV10 Catalogue name (NAME_vv10)
meta.id
char
typevv10
[B/A/Q] VV10 Object type (Type_vv10)
src.class
char
vmagvv10
? VV10 V magnitude (Vmag_vv10)
mag
phot.mag;em.opt.V
double
zvv10
? VV10 Redshift (z_vv10)
src.redshift;pos.heliocentric
double
indexvv10
? VV10 Running catalogue number (Index_vv10) (157)
meta.id
int
ra5deg
VV10 Right ascension (J2000) (RA_vv10)
deg
pos.eq.ra
double
de5deg
VV10 Declination (J2000) (DEC_vv10)
deg
pos.eq.dec
double
mtyc2
? Number of the nearest counterpart in the Tycho2 Catalogue (mult_tyc2)
meta.number
short
etyc2
? Source number of nearest Tyc2 counterpart (entr_tyc2)
meta.id
int
dtyc2
?=0 Distance to nearest Tyc2 counterpart (dist_tyc2) (162)
arcsec
pos.angDistance;src.orbital
double
ra6deg
Tyc2 Right ascension (J2000) (RA_tyc2)
deg
pos.eq.ra
double
de6deg
Tyc2 Declination (J2000) (DEC_tyc2)
deg
pos.eq.dec
double
recnotyc2
? Tyc2 Catalogue number (RecNo_tyc2)
meta.id
int
vtmag
? Tyc2 VT magnitude (VTmag_tyc2) (6)
mag
phot.mag;em.opt.V
double
btmag
? Tyc2 BT magnitude (BTmag_tyc2) (6)
mag
phot.mag;em.opt.B
double
tyc1
? Tyc2 TYC1 number (TYC1_tyc2) (7)
meta.id
short
tyc2
? Tyc2 TYC2 number (TYC2_tyc2) (7)
meta.id
int
tyc3
? Tyc2 TYC3 number (TYC3_tyc2) (7)
meta.id
short
mbsc
? Number of counterparts in the Catalogue of Bright Stars (BSC) within the distance of 300" (mult_bri)
meta.number
short
ebsc
? Source number of nearest BSC counterpart (entr_bri)
meta.id
short
dbsc
?=0 Distance to nearest BSC counterpart (dist_bri)
arcsec
pos.angDistance;src.orbital
double
ra7deg
BSC Right ascension (J2000) (RA_bri)
deg
pos.eq.ra
double
de7deg
BSC Declination (J2000) (DEC_bri)
deg
pos.eq.dec
double
vmagbsc
? BSC V magnitude (Vmag_bri)
mag
phot.mag;em.opt.V
double
sptypebsc
BSC spectral type (SpType_bri)
src.spType
char
recnobsc
? BSC Record catalogue number (RecNo_bri)
meta.id
short
hd
? Henry Draper Catalogue Number (HD_bri)
meta.id
int
mhmxb
? Number of counterparts in the Catalog of High Mass X-Ray Binaries (HMXBCAT) within the distance of 60" (mult_hmxb)
meta.number
short
ehmxb
? Source number of nearest HMXBCAT counterpart (entr_hmxb)
meta.id
short
dhmxb
?=0 Distance of nearest HMXBCAT counterpart (dist_hmxb)
arcsec
pos.angDistance;src.orbital
double
ra8deg
HMXBCAT Right ascension (J2000) (RA_hmxb)
deg
pos.eq.ra
double
de8deg
HMXBCAT Declination (J2000) (DEC_hmxb)
deg
pos.eq.dec
double
namehmxb
HMXBCAT Catalogue name (Name_hmxb)
meta.id
char
name2hmxb
HMXBCAT Alternative catalogue name (Name2_hmxb)
meta.id
char
vmaghmxb
? HMXBCAT V magnitude (Vmag_hmxb)
mag
phot.mag;em.opt.V
double
mlmxb
? Number of counterparts in the Catalog of Low Mass X-Ray Binaries (LMXBCAT) within the distance of 60" (mult_lmxb)
meta.number
short
elmxb
? Source number of nearest LMXBCAT counterpart (entr_lmxb)
meta.id
short
dlmxb
?=0 Distance to nearest LMXBCAT counterpart (dist_lmxb)
arcsec
pos.angDistance;src.orbital
double
ra9deg
LMXBCAT Right ascension (J2000) (RA_lmxb)
deg
pos.eq.ra
double
de9deg
LMXBCAT Declination (J2000) (DEC_lmxb)
deg
pos.eq.dec
double
namelmxb
LMXBCAT Catalogue name (Name_lmxb)
meta.id
char
name2lmxb
LMXBCAT Alternative catalogue name (Name2_lmxb) (194)
meta.id
char
vmaglmxb
? LMXBCAT V magnitude (Vmag_lmxb)
mag
phot.mag;em.opt.V
double
matnf
? Number of counterparts in the Pulsar Catalogue (ATNF) within the distance of 60" (mult_atnf)
meta.number
short
eatnf
? Source number of nearest ATNF counterpart (entr_atnf)
meta.id
short
datnf
?=0 Distance to nearest ATNF counterpart (dist_atnf)
arcsec
pos.angDistance;src.orbital
double
ra10deg
ATNF Right ascension (J2000) (RA_atnf)
deg
pos.eq.ra
double
de10deg
ATNF Declination (J2000) (DEC_atnf)
deg
pos.eq.dec
double
atnf
ATNF Pulsar name (Name_atnf)
meta.id
char
typeatnf
ATNF Pulsar type (Type_atnf)
src.class
char
peratnf
ATNF Pulsar period (Period_atnf)
s
time.period
char
mfuh
? Number of counterparts in the Catalog of Variable Sources from Fuhrmeister and Schmitt within the distance of 60" (mult_fuh)
meta.number
short
efuh
? Source number of nearest FUH counterpart (entr_fuh)
meta.id
short
dfuh
?=0 Distance to nearest FUH counterpart (dist_fuh)
arcsec
pos.angDistance;src.orbital
double
ra11deg
FUH Right ascension (J2000) (RA_fuh)
deg
pos.eq.ra
double
de11deg
FUH Declination (J2000) (DEC_fuh)
deg
pos.eq.dec
double
seqfuh
FUH Object number (Seq_fuh)
meta.id
char
namefuh
FUH Object name (Name_fuh)
meta.id
char
m1sxps
? Number of counterparts in Swift 1SXPS catalogue within a distance of 120" (mult_1sxps)
meta.number
short
e1sxps
? Source number of nearest 1SXPS counterpart (entr_1sxps)
meta.id
int
d1sxps
?=0 Distance to nearest 1SXPS counterparts (dist_1sxps)
arcsec
pos.angDistance;src.orbital
double
ra12deg
1SXPS Right ascension (J2000) (RA_1sxps)
deg
pos.eq.ra
double
de12deg
1SXPS Declination (J2000) (DEC_1sxps)
deg
pos.eq.dec
double
exp1sxps
? 1SXPS Source exposure time (Expos_1sxps)
s
time.duration;obs.exposure
int
det1sxps
? 1SXPS Total(0.3-10keV)-band detection flag (DET_1sxps)
meta.code
short
det01sxps
? 1SXPS Total(0.3-10keV)-band detection flag (DET0_1sxps)
meta.code
short
det11sxps
? 1SXPS Soft(0.3-1keV)-band detection flag (DET1_1sxps)
meta.code
short
det21sxps
? 1SXPS Meduin(2-2keV)-band detection flag (DET2_1sxps)
meta.code
short
det31sxps
? 1SXPS Hard(2-10keV)-band detection flag (DET3_1sxps)
meta.code
short
"1sxps"
? Running catalogue number in Swift (INDEX_1sxps)
meta.id
char
cr01sxps
? Swift Total (0.3-10 keV)-band count rate (Rate0_1sxps)
ct/s
phot.count;em.X-ray
double
e_cr01sxps
? Swift Error of Rate0_1sxps (ERate0_1sxps)
ct/s
stat.error
double
m1rxh
? Number of counterparts in the 1RXH catalogue within the distance of 120" (mult_1rxh)
meta.number
short
e1rxh
? Source number of nearest 1RXH counterpart (entr_1rxh)
meta.id
int
d1rxh
?=0 Distance to nearest 1RXH counterpart (dist_1rxh)
arcsec
pos.angDistance;src.orbital
double
ra13deg
1RXH Right ascension (J2000) (RA_1rxh)
deg
pos.eq.ra
double
de13deg
1RXH Declination (J2000) (DEC_1rxh)
deg
pos.eq.dec
double
"1rxh"
Source name in the 1RXH (SRCNAME_1rxh)
meta.id
char
cr1rxh
? 1RXH Source count rate (CRATE_1rxh)
ct/s
phot.count;em.X-ray
double
e_cr1rxh
? Error of CRATE_1RXH (CRATE_err_1rxh)
ct/s
stat.error
double
etim1rxh
? 1RXH Source exposure time (ExpTime_1rxh)
s
time.duration;obs.exposure
int
snr1rxh
? 1RXH Signal-to-noise ratio (SNR_1rxh)
stat.snr
double
mflem
? Number of counterparts in the Catalog of White Dwarfs from Flemming within the distance of 60" (mult_flem)
meta.number
short
eflem
? Source number of nearest Flemming counterpart (entr_flem)
meta.id
short
dflem
?=0 Distance to nearest Flemming counterpart (dist_flem)
arcsec
pos.angDistance;src.orbital
double
ra14deg
Flemming Right ascension (J2000) (RA_flem)
deg
pos.eq.ra
double
de14deg
Flemming Declination (J2000) (DEC_flem)
deg
pos.eq.dec
double
flem
Source name in the Flemming Catalogue (SRCNAME_flem)
meta.id
char
typeflem
Flemming Object type (Type_flem)
src.class
char
wfcflem
[Y/N] Flemming Wide Field Camera detection? (WFC_flem)
meta.code
char
crflem
? Flemming count rate (Rate_flem)
ct/s
phot.count;em.X-ray
double
e_crflem
? Error of the Flemming count rate (e_Rate_flem)
ct/s
stat.error
double
mwd
? Number of counterparts in the Catalog of White Dwarfs within the distance of 60 " (mult_wd)
meta.number
short
ewd
? Source number of nearest WD counterpart (entr_wd)
meta.id
int
dwd
?=0 Distance to nearest WD counterpart (dist_wd)
arcsec
pos.angDistance;src.orbital
double
ra15deg
WD Rigth ascension (J2000) (RA_wd)
deg
pos.eq.ra
double
de15deg
WD Declination (J2000) (DEC_wd)
deg
pos.eq.dec
double
wd
WD Source name in the Catalogue (SRCNAME_wd)
meta.id
char
vmagwd
? WD V-magnitude (Vmag_wd)
mag
phot.mag;em.opt.V
double
vsphotwd
? WD V mag: multichannel spectrophotometry (Vsphot_wd)
mag
phot.mag;em.opt.V
double
msdss
? Source number of the nearest counterpart in the Sloan Catalogue (mult_sdss)
meta.number
short
esdss
? Source number of SDSS nearest counterpart (entr_sdss)
meta.id
short
dsdss
?=0 Distance to nearest SDSS counterpart (dist_sdss)
arcsec
pos.angDistance;src.orbital
double
ra16deg
SDSS Right ascension (J2000) (RA_sdss)
deg
pos.eq.ra
double
de16deg
SDSS Declination (J2000) (DEC_sdss)
deg
pos.eq.dec
double
sdss
SDSS Object name (SDSS_NAME)
meta.id
char
lambdas
? SDSS Latitude in elliptical coordinate (LAMBDA_sdss)
deg
pos.ecliptic.lat
double
betas
? SDSS Longitude in elliptical coordinate (BETA_sdss)
deg
pos.ecliptic.lon
double
m2rxs
? Number of counterparts in the 2RXS catalogue within the distance of 60" (mult_2rxs)
meta.number
short
e2rxs
? Source number of 2RXS counterpart (entr_2rxs)
meta.id
int
d2rxs
?=0 Distance to 2RXS counterpart (dist_2rxs)
arcsec
pos.angDistance;src.orbital
double
i2rxs
? Index of the nearest 2RXS counterpart (INDEX_2rxs)
meta.id
int
seq2rxs
? Number of sky field of 2RXS nearest counterpart (SEQ_ID_2rxs)
meta.id;obs.field
int
indd2rxs
? Field detection number of 2RXS nearest counterpart (IND_DET_2rxs)
meta.id;obs.field
short
eximl2rxs
? Detection likelihood of 2RXS nearest counterpart (EXI_ML_2rxs)
stat.likelihood
double
cr2rxs
? Source count rate of 2RXS nearest counterpart (RATE_2rxs)
ct/s
phot.count;em.X-ray
double
ra17deg
2RXS Right ascension (J2000) (RA_2rxs)
deg
pos.eq.ra
double
de17deg
2RXS Declination (J2000) (DEC_2rxs)
deg
pos.eq.dec
double
usky2rxs
[-1/9]? Sub-field detection cell of 2RXS nearest counterpart (USKY_2rxs)
meta.code
short
flag2rxs
[0/1]? Nearby flag of 2RXS nearest counterpart, 0=best (FLAG_2rxs)
meta.code.error
short
bkgid
? Selected background (BKG_id)
meta.code
short
xbkg1
? X_sky coordinate of background center 1 in sky pixel (X_BKG_1)
pix
pos.cartesian.x;instr.det
double
ybkg1
? Y_sky coordinate of background center 1 in sky pixel (Y_BKG_1)
pix
pos.cartesian.y;instr.det
double
xbkg2
? X_sky coordinate of background center 2 in sky pixel (X_BKG_2)
pix
pos.cartesian.x;instr.det
double
ybkg2
? Y_sky coordinate of background center 2 in sky pixel (Y_BKG_2)
pix
pos.cartesian.y;instr.det
double
bgr1rxs
? Background count rate per square arcmin from 1RXS (BGR_1rxs)
ct/s/arcmin2
arith.rate;instr.background
double
bgr2rxs
Background count rate per square arcmin from 2RXS (BGR_2rxs)
ct/s/arcmin2
arith.rate;instr.background
double
lflag
? Variability flag 0=good,1=bkg (LFLAG) (8)
meta.code;src.var
short
cm6
? Count rate for light curve with less than 6s exposure (CM6)
ct/s
phot.count;em.X-ray
double
cd6
? Standard deviation of light curves with less than 6s exposure (CD6)
ct/s
stat.error
double
exvar6
? Excess variance for light curves with less than 6s exposure (EXCESSVAR6)
stat.variance
double
e_exvar6
? Excess variance uncertainty (UNCERTAINTY6)
stat.error
double
nbinsa
? Number of data points in the LC (NBINS_A)
meta.number
short
nbins6
? Number of data points with exposures times less than 6s (NBINS_6)
meta.number
short
nbins1
? Number of data points with exposures times less than 1s (NBINS_1)
meta.number
short
nbinsn
? Number of data points with exposure times greater than 6s (NBINS_N)
meta.number
short
cmin6
? Minimum count rate for light curves with exposure times of less than 6s (CMIN6)
ct/s
phot.count;em.X-ray
double
cmax6
? Maximum count rate for light curves with exposure times of less than 6s (CMAX6)
ct/s
phot.count;em.X-ray
double
e_cmin6
? Error of CMIN6 (EMIN6)
ct/s
stat.error
double
e_cmax6
? Error of CMAX6 (EMAX6)
ct/s
stat.error
double
ctslc6
[-]? Number of counts for light curves with exposure times of less than 6s (CTS_lc6) Not used
ct
phot.count
double
sigex6
? Excess variance for light curves with exposure times of less than 6s (SIGMA_excess6)
stat.variance
double
"cm+cd"
? Sum of count rate + standard deviation
stat.fit.param
double
spx
[0/1] graphical illustrations from spectral fits available in spx subdirectory
meta.code
char
lcx
[0/1] light curve exists as graphical illustration in clx subdirectory
meta.code
char
obsclock1
? Start time of exposure when source is within FOV and detector ons (OBS_CLOCK_1)
s
time.start;obs.exposure
double
obsclock2
? End time of exposure when source is within FOV and detector ons (OBS_CLOCK_2)
s
time.end;obs.exposure
double
obs_date1
? Start time of exposure when source is within FOV and detector on (OBS_DATE_1)
"Y:M:D"
time.start;obs.exposure
double
obs_time1
? Start time (OBS_UT_1)
deg
time.epoch
double
obs_date2
? End time of exposure when source is within FOV and detector on (OBS_DATE_2)
"Y:M:D"
time.end;obs.exposure
double
obs_time2
? End time (OBS_UT_2)
deg
time.epoch
double
catalogues.mv_cat2sxps_sources_fdw
cat2sxps_sources_oid
null
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
"2SXPS_ID"
meta.id;meta.main
int
primary
IAUName
char
primary
RA
The Right Ascension (J2000) of the source, taken from the individual detection with the highest S/N and best detection flag.
deg
pos.eq.ra;meta.main
double
primary
Decl
The declination (J2000) of the source, taken from the individual detection with the highest S/N and best detection flag.
deg
pos.eq.dec;meta.main
double
primary
Err90
The 90% confidence radial position error on the source position, taken from the same individual detection as the position. This includes the astrometric systematic error.
double
AstromType
This relates the provenance of the astrometry used to derive the source position.
short
l
double
b
double
MeanOffAxisAngle
The mean distance angle (in arc minutes) of the source from the centre of the XRT detector averaged over all observations in which the source was detected and inside the XRT field of view. There is a handful of sources for which this value is -1. This indicates that the source centre was never in the field of view, that is, the detection and centroid was based on the wings of the PSF that extended into the field of view while the source itself was outside.
double
OrigErr90
In the initial release of 2SXPS the statsitical component of the error was a factor of 1.5 too large, due to an error in the conversion from 1-σ to 90% confidence. This has now been corrected, however the value originally released (and used in cross correlation) is given in this field.
double
NearestNeighbour
The distance to the nearest 2SXPS source to this one, in arcsec.
double
NearestOKNeighbour
The distance to the nearest 2SXPS source to this one, with a flag of 0 or 1, i.e. Good or Reasonable with no other warning bit set; in arcsec.
double
Exposure
The total exposure at the location of the source in seconds, including datasets in which the source was not detected.
int
FirstObsDate
The UTC date and time of the start of the first observation in 2SXPS which covered the location of the source.
iso-8601
TIME
char
LastObsDate
The UTC date and time of the end of the last observation in 2SXPS which covered the location of the source.
iso-8601
TIME
char
FirstObsMET
The time of the start of the first observation in 2SXPS which covered the location of the source, in Swift MET.
int
LastObsMET
The time of the end of the last observation in 2SXPS which covered the location of the source, in Swift MET.
int
FirstDetDate
The UTC date and time of the start of the first observation in 2SXPS in which the source count-rate in any band is inconsistent with 0 at the 3-σ level; i.e. the first observation in which the source was detected by the blind search or retrospective count-rate determination.
iso-8601
TIME
char
LastDetDate
The UTC date and time of the end of the last observation in 2SXPS in which the source count-rate in any band is inconsistent with 0 at the 3-σ level; i.e. the first observation in which the source was detected by the blind search or retrospective count-rate determination.
iso-8601
TIME
char
FirstDetMET
The time, in Swift MET, of the start of the first observation in 2SXPS in which the source count-rate in any band is inconsistent with 0 at the 3-σ level; i.e. the first observation in which the source was detected by the blind search or retrospective count-rate determination.
int
LastDetMET
The time, in Swift MET, of the end of the last observation in 2SXPS in which the source count-rate in any band is inconsistent with 0 at the 3-σ level; i.e. the first observation in which the source was detected by the blind search or retrospective count-rate determination.
int
FirstBlindDetDate
The UTC date and time of the start of the first observation in 2SXPS in which the source was detected in the blind search.
iso-8601
TIME
char
LastBlindDetDate
The UTC date and time of the end of the last observation in 2SXPS in in which the source was detected in the blind search.
iso-8601
TIME
char
FirstBlindDetMET
The time, in Swift MET, of the start of the first observation in 2SXPS in which the source was detected in the blind search.
int
LastBlindDetMET
The time, in Swift MET, of the end of the last observation in 2SXPS in which the source was detected in the blind search.
int
NumObs
The total number of datasets (observations+stacked images) which cover the location of the source, including those in which the source was not detected.
short
NumBlindDetObs
The number of datasets (observations+stacked images) in which the source was detected in the blind search.
short
NumDetObs
The number of datasets (observations+stacked images) in which the source was detected with the retrospective analysis.
short
BestDetectionID
The ID value from the detections table corresponding to the detection of this source for which the position and error have been taken.
int
NonBlindDet_band0
Whether the mean count-rate in the total (0.3—10 keV) is non-zero with 3-σ significance.
short
NonBlindDet_band1
Whether the mean count-rate in the soft (0.3—1 keV) is non-zero with 3-σ significance.
short
NonBlindDet_band2
Whether the mean count-rate in the medium (1—2 keV) is non-zero with 3-σ significance.
short
NonBlindDet_band3
Whether the mean count-rate in the hard (3—10 keV) is non-zero with 3-σ significance.
short
DetFlag
The best detection flag from all detections of the source. The basic values are 0, 1, or 2, meaning Good, Reasonable or Poor respectively. Higher values mean that an extra warning is associated with the source.
short
primary
FieldFlag
short
DetFlag_band0
The best total-band (0.3—10 keV) detection flag from all detections of the source.
short
DetFlag_band1
The best soft-band (0.3—1 keV) detection flag from all detections of the source.
short
DetFlag_band2
The best medium-band (1—2 keV) detection flag from all detections of the source.
short
DetFlag_band3
The best hard-band (2—10 keV) detection flag from all detections of the source.
short
OpticalLoadingWarning
This is the worst optical loading warning from any detection of the source. If an optical source exists near the 2SXPS source, and is bright enough to cause optical loading then this field indicates how many magnitudes brighter than the optical loading limit that source is, otherwise it is zero.
double
StrayLightWarning
This is set to one if any detections of the source occurred in a region affected by stray light, otherwise zero.
short
NearBrightSourceWarning
Whether any detection of this source occurred where the background level exceeded 10-3 ct s-1 pixel-1, i.e. was likely in the wings of a bright source. A value of zero indicates this did not occur. A value of one indicates that it did. A value of two means that the source was detected in a stacked image in which the background was not high (averaged over the whole stacked exposure), but where there was at least one observation in which the source was undetected, and the background at the source position was in excess of 10-3 ct s-1 pixel-1.
short
IsPotentialAlias
short
PotentialAliasList
char
Rate_band0
The time-averaged total-band (0.3—10 keV) count-rate of the source, in counts per second.
ct/s
double
primary
Rate_band0_pos
The 1-σ positive error on the time-averaged total-band (0.3—10 keV) count-rate of the source. If more than 100 net counts (i.e. after background subtraction) were detected, or the number of counts in the source or background exceeded 1000, this is the Poisson error, otherwise it is calculated from the Bayesian method of Kraft, Burrows & Nousek (1991).
ct/s
double
primary
Rate_band0_neg
The 1-σ negative error on the time-averaged total-band (0.3—10 keV) count-rate of the source. If more than 100 net counts (i.e. after background subtraction) were detected, or the number of counts in the source or background exceeded 1000, this is the Poisson error, otherwise it is calculated from the Bayesian method of Kraft, Burrows & Nousek (1991).
ct/s
double
primary
HR1
The HR1 hardness ratio = (M-S)/(M+S) where M and S are the medium (1—2 keV) and soft (0.3—1 keV) band count-rates. If both bands had more than 100 photons and an S/N ratio of at least 2 this was calculated simply from this equation, otherwise the Bayesian approach of Park et al. (2006) was employed.
double
primary
HR1_pos
The 1-σ positive error on HR1. In a small number of cases where the Bayesian approach of Park et al. (2006) was used to derive HR1, the mean HR value lay outside the 1-σ confidence interval. In these cases the HR1_pos error may be negative.
double
HR1_neg
The 1-σ negative error on HR1. In a small number of cases where the Bayesian approach of Park et al. (2006) was used to derive HR1, the mean HR value lay outside the 1-σ confidence interval. In these cases the HR1_neg error may be positive.
double
HR2
The HR2 hardness ratio = (H-M)/(H+M) where H and M are the hard (2—10 keV) and medium (1—2 keV) band count-rates. If both bands had more than 100 photons and an SNR of at least 2 this was calculated simply from this equation, otherwise the Bayesian approach of Park et al. (2006) was employed.
double
primary
HR2_pos
The 1-σ positive error on HR2. In a small number of cases where the Bayesian approach of Park et al. (2006) was used to derive HR2, the mean HR value lay outside the 1-σ confidence interval. In these cases the HR2_pos error may be negative.
double
HR2_neg
The 1-σ negative error on HR2. In a small number of cases where the Bayesian approach of Park et al. (2006) was used to derive HR2, the mean HR value lay outside the 1-σ confidence interval. In these cases the HR2_neg error may be positive.
double
Rate_band1
The time-averaged soft-band (0.3—1 keV) count-rate of the source, in counts per second.
double
Rate_band1_pos
The 1-σ positive error on the time-averaged soft-band (0.3—1 keV) count-rate of the source.
double
Rate_band1_neg
The 1-σ negative error on the time-averaged soft-band (0.3—1 keV) count-rate of the source.
double
Rate_band2
The time-averaged medium-band (1—2 keV) count-rate of the source, in counts per second.
double
Rate_band2_pos
The 1-σ positive error on the time-averaged medium-band (1—2 keV) count-rate of the source.
double
Rate_band2_neg
The 1-σ negative error on the time-averaged medium-band (1—2 keV) count-rate of the source.
double
Rate_band3
The time-averaged hard-band (2—10 keV) count-rate of the source, in counts per second.
double
Rate_band3_pos
The 1-σ positive error on the time-averaged hard-band (2—10 keV) count-rate of the source.
double
Rate_band3_neg
The 1-σ negative error on the time-averaged hard-band (2—10 keV) count-rate of the source.
double
Counts_band0
The total number of events (not background subtracted or exposure corrected) in the total-band (0.3—10 keV) image, in the source extraction region for this source. This is found by summing the counts in the individual observations of the location, not from the stacked image.
int
Counts_band1
The total number of events (not background subtracted or exposure corrected) in the soft-band (0.3—1 keV) image, in the source extraction region for this source.
int
Counts_band2
The total number of events (not background subtracted or exposure corrected) in the medium-band (1—2 keV) image, in the source extraction region for this source.
int
Counts_band3
The total number of events (not background subtracted or exposure corrected) in the hard-band (2—10 keV) image, in the source extraction region for this source.
int
BgCounts_band0
double
BgCounts_band1
double
BgCounts_band2
double
BgCounts_band3
double
RateCF_band0
The count-rate correction factor in the total band (0.3—10 keV). This corrects for vignetting, bad columns, pile-up and the finite radius within which counts were extracted.
double
RateCF_band1
The count-rate correction factor in the soft band (0.3—1 keV).
double
RateCF_band2
The count-rate correction factor in the medium band (1—2 keV).
double
RateCF_band3
The count-rate correction factor in the hard band (2—10 keV).
double
UL_band0
The overall 3-σ upper limit on the total-band (0.3—10 keV) count-rate from the source, derived from the Counts_band0, BGCounts_band0, RateCF_band0 and Exposure columns. If more than 100 net counts (i.e. after background subtraction) were detected, or the number of counts in the source or background exceeded 1000, this was determined using Poisson errors, otherwise it is calculated from the Bayesian method of Kraft, Burrows & Nousek (1991). Note that this upper limit value is supplied for all sources, regardless of the strength of the detection.
double
UL_band1
The overall 3-σ upper limit on the soft-band (0.3—1 keV) count-rate from the source.
double
UL_band2
The overall 3-σ upper limit on the medium-band (1—2 keV) count-rate from the source.
double
UL_band3
The overall 3-σ upper limit on the hard-band (2—10 keV) count-rate from the source.
double
PeakRate_band0
The peak count-rate of the source in the total band (0.3—10 keV). The peak rate is defined as the count-rate in the light curve bin (from per-snapshot or per-obsid binning) with the highest 1-σ lower limit.
double
PeakRate_band0_pos
The 1-σ positive error on the peak total-band (0.3—10 keV) count-rate of the source.
double
PeakRate_band0_neg
The 1-σ negative error on the peak total-band (0.3—10 keV) count-rate of the source.
double
PeakRate_band1
The peak count-rate of the source in the soft band (0.3—1 keV).
double
PeakRate_band1_pos
The 1-σ positive error on the peak total-band (0.3—1 keV) count-rate of the source.
double
PeakRate_band1_neg
The 1-σ negative error on the peak total-band (0.3—1 keV) count-rate of the source.
double
PeakRate_band2
The peak count-rate of the source in the soft band (1—2 keV).
double
PeakRate_band2_pos
The 1-σ positive error on the peak total-band (1—2 keV) count-rate of the source.
double
PeakRate_band2_neg
The 1-σ negative error on the peak total-band (1—3 keV) count-rate of the source.
double
PeakRate_band3
The peak count-rate of the source in the soft band (2—10 keV).
double
PeakRate_band3_pos
The 1-σ positive error on the peak total-band (2—10 keV) count-rate of the source.
double
PeakRate_band3_neg
The 1-σ negative error on the peak total-band (2—10 keV) count-rate of the source.
double
GalacticNH
The Galactic absorption column density (in cm-2) in the direction of the source, determined from Willingale et al. (2013).
double
PvarPchiSnapshot_band0
The probability that the source is constant between snapshots in the total band (0.3—10 keV), as derived from the Pearsons χ2 test. The minimum recordable value for this is 1.1×10-16 so values of 0 mean <1.1×10-16.
double
primary
PvarPchiSnapshot_band1
The probability that the source is constant between snapshots in the soft band (0.3—1 keV), as derived from the Pearsons χ2 test.
double
PvarPchiSnapshot_band2
The probability that the source is constant between snapshots in the medium band (1—2 keV), as derived from the Pearsons χ2 test.
double
PvarPchiSnapshot_band3
The probability that the source is constant between snapshots in the hard band (2—10 keV), as derived from the Pearsons χ2 test.
double
PvarPchiSnapshot_HR1
The probability that the source HR1 hardness ratio is constant between snapshots, as derived from the Pearsons χ2 test.
double
PvarPchiSnapshot_HR2
The probability that the source HR2 hardness ratio is constant between snapshots, as derived from the Pearsons χ2 test.
double
PvarPchiObsID_band0
The probability that the source is constant between observations in the total band (0.3—10 keV), as derived from the Pearsons χ2 test.
double
PvarPchiObsID_band1
The probability that the source is constant between observations in the soft band (0.3—1 keV), as derived from the Pearsons χ2 test.
double
PvarPchiObsID_band2
The probability that the source is constant between observations in the medium band (1—2 keV), as derived from the Pearsons χ2 test.
double
PvarPchiObsID_band3
The probability that the source is constant between observations in the hard band (2—10 keV), as derived from the Pearsons χ2 test.
double
PvarPchiObsID_HR1
The probability that the source HR1 hardness ratio is constant between observations, as derived from the Pearsons χ2 test.
double
PvarPchiObsID_HR2
The probability that the source HR2 hardness ratio is constant between observations, as derived from the Pearsons χ2 test.
double
WhichPow
TheWhich method of determining the spectral properties assuming a power-law was used
short
WhichAPEC
Which method of determining the spectral properties assuming an APEC was used
short
PowECFO
The counts-to-observed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from the power-law spectrum indicated by the WhichPow field.
double
PowECFU
The counts-to-unabsorbed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from the power-law spectrum indicated by the WhichPow field.
double
PowFlux
The observed 0.3—10 keV flux (in erg cm-2 s-1) derived from the power-law spectrum indicated by the WhichPow field. This is given by Rate_band0*PowECFO.
mW/m2
double
primary
PowFlux_pos
The 1-σ positive error on the observed 0.3—10 keV flux for the power-law spectrum indicated by the WhichPow field. This is given by Rate_band0_pos*PowECFO, so does not include uncertainties in the spectral modelling.
double
PowFlux_neg
The 1-σ negative error on the observed 0.3—10 keV flux for the power-law spectrum indicated by the WhichPow field. This is given by Rate_band0_neg*PowECFO, so does not include uncertainties in the spectral modelling.
double
PowUnabsFlux
The unabsorbed 0.3—10 keV flux (in erg cm-2 s-1), derived from the power-law spectrum indicated by the WhichPow field. This is given by Rate_band0*PowECFU.
mW/m2
double
primary
PowUnabsFlux_pos
The 1-σ positive error on the unabsorbed 0.3—10 keV flux for the power-law spectrum indicated by the WhichPow field. This is given by Rate_band0_pos*PowECFU, so does not include uncertainties in the spectral modelling.
double
PowUnabsFlux_neg
The 1-σ negative error on the unabsorbed 0.3—10 keV flux for the power-law spectrum indicated by the WhichPow field. This is given by Rate_band0_neg*PowECFU, so does not include uncertainties in the spectral modelling.
double
APECECFO
The counts-to-observed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived the APEC spectrum indicated by the WhichAPEC field.
double
APECECFU
The counts-to-unabsorbed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from the APEC spectrum indicated by the WhichAPEC field.
double
APECFlux
The observed 0.3—10 keV flux (in erg cm-2 s-1) derived from the APEC spectrum indicated by the WhichAPEC field. This is given by Rate_band0*APECECFO.
double
APECFlux_pos
The 1-σ positive error on the observed 0.3—10 keV flux for the APEC spectrum indicated by the WhichAPEC field. This is given by Rate_band0_pos*APECECFO, so does not include uncertainties in the spectral modelling.
double
APECFlux_neg
The 1-σ negative error on the observed 0.3—10 keV flux for the APEC spectrum indicated by the WhichAPEC field. This is given by Rate_band0_neg*APECECFO, so does not include uncertainties in the spectral modelling.
double
APECUnabsFlux
The unabsorbed 0.3—10 keV flux (in erg cm-2 s-1), derived from the APEC spectrum indicated by the WhichAPEC field. This is given by Rate_band0*APECECFU.
double
APECUnabsFlux_pos
The 1-σ positive error on the unabsorbed 0.3—10 keV flux for the APEC spectrum indicated by the WhichAPEC field. This is given by Rate_band0_pos*APECECFU, so does not include uncertainties in the spectral modelling.
double
APECUnabsFlux_neg
The 1-σ negative error on the unabsorbed 0.3—10 keV flux for the APEC spectrum indicated by the WhichAPEC field. This is given by Rate_band0_neg*APECECFU, so does not include uncertainties in the spectral modelling.
double
PowPeakFlux
The peak observed 0.3—10 keV flux (in erg cm-2 s-1) for the power-law spectrum indicated by the WhichPow field. This is given by PeakRate_band0*PowECFO.
double
PowPeakFlux_pos
The 1-σ positive error on the peak observed 0.3—10 keV flux for the power-law spectrum indicated by the WhichPow field. This is given by PeakRate_band0_pos*PowECFO, so does not include uncertainties in the spectral modelling.
double
PowPeakFlux_neg
The 1-σ negative error on the peak observed 0.3—10 keV flux for the power-law spectrum indicated by the WhichPow field. This is given by PeakRate_band0_neg*PowECFO, so does not include uncertainties in the spectral modelling.
double
PowPeakUnabsFlux
The peak unabsorbed 0.3—10 keV flux (in erg cm-2 s-1) for the power-law spectrum indicated by the WhichPow field. This is given by PeakRate_band0*PowECFU.
double
PowPeakUnabsFlux_pos
The 1-σ positive error on the peak unabsorbed 0.3—10 keV flux for the power-law spectrum indicated by the WhichPow field. This is given by PeakRate_band0_pos*PowECFU, so does not include uncertainties in the spectral modelling.
double
PowPeakUnabsFlux_neg
The 1-σ negative error on the peak unabsorbed 0.3—10 keV flux for the power-law spectrum indicated by the WhichPow field. This is given by PeakRate_band0_neg*PowECFU, so does not include uncertainties in the spectral modelling.
double
APECPeakFlux
The peak observed 0.3—10 keV flux (in erg cm-2 s-1) for the APEC spectrum indicated by the WhichAPEC field. This is given by PeakRate_band0*APECECFO.
double
APECPeakFlux_pos
The 1-σ positive error on the peak observed 0.3—10 keV flux for the APEC spectrum indicated by the WhichAPEC field. This is given by PeakRate_band0_pos*APECECFO, so does not include uncertainties in the spectral modelling.
double
APECPeakFlux_neg
The 1-σ negative error on the peak observed 0.3—10 keV flux for the APEC spectrum indicated by the WhichAPEC field. This is given by PeakRate_band0_neg*APECECFO, so does not include uncertainties in the spectral modelling.
double
APECPeakUnabsFlux
The peak unabsorbed 0.3—10 keV flux (in erg cm-2 s-1) for the APEC spectrum indicated by the WhichAPEC field. This is given by PeakRate_band0*APECECFU.
double
APECPeakUnabsFlux_pos
The 1-σ positive error on the peak unabsorbed 0.3—10 keV flux for the APEC spectrum indicated by the WhichAPEC field. This is given by PeakRate_band0_pos*APECECFU, so does not include uncertainties in the spectral modelling.
double
APECPeakUnabsFlux_neg
The 1-σ negative error on the peak unabsorbed 0.3—10 keV flux for the APEC spectrum indicated by the WhichAPEC field. This is given by PeakRate_band0_neg*APECECFU, so does not include uncertainties in the spectral modelling.
double
FixedPowECFO
The counts-to-observed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from a power-law spectrum with a photon index of 1.7 absorbed by the Galactic column (from the GalacticNH field).
double
FixedPowECFU
The counts-to-unabsorbed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from a power-law spectrum with a photon index of 1.7 absorbed by the Galactic column (from the GalacticNH field).
double
FixedPowFlux
The observed 0.3—10 keV flux (in erg cm-2 s-1) derived from a power-law spectrum with a photon index of 1.7 absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0*FixedPowECFO.
double
FixedPowFlux_pos
The 1-σ positive error on the observed 0.3—10 keV flux for a power-law spectrum with a photon index of 1.7 absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0_pos*FixedPowECFO, so does not include uncertainties in the spectral modelling.
double
FixedPowFlux_neg
The 1-σ negative error on the observed 0.3—10 keV flux for a power-law spectrum with a photon index of 1.7 absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0_neg*FixedPowECFO, so does not include uncertainties in the spectral modelling.
double
FixedPowUnabsFlux
The unabsorbed 0.3—10 keV flux (in erg cm-2 s-1) derived from a power-law spectrum with a photon index of 1.7 absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0*FixedPowECFU.
double
FixedPowUnabsFlux_pos
The 1-σ positive error on the unabsorbed 0.3—10 keV flux for a power-law spectrum with a photon index of 1.7 absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0_pos*FixedPowECFU, so does not include uncertainties in the spectral modelling.
double
FixedPowUnabsFlux_neg
The 1-σ negative error on the unabsorbed 0.3—10 keV flux for a power-law spectrum with a photon index of 1.7 absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0_neg*FixedPowECFU, so does not include uncertainties in the spectral modelling.
double
FixedAPECECFO
The counts-to-observed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from an APEC spectrum with a temperature of 1 keV absorbed by the Galactic column (from the GalacticNH field).
double
FixedAPECECFU
The counts-to-unabsorbed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from an APEC spectrum with a temperature of 1 keV absorbed by the Galactic column (from the GalacticNH field).
double
FixedAPECFlux
The observed 0.3—10 keV flux (in erg cm-2 s-1) derived from an APEC spectrum with a temperature of 1 keV absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0*FixedAPEECECFO.
double
FixedAPECFlux_pos
The 1-σ positive error on the observed 0.3—10 keV flux for an APEC spectrum with a temperature of 1 keV absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0_pos*FixedAPECECFO, so does not include uncertainties in the spectral modelling.
double
FixedAPECFlux_neg
The 1-σ negative error on the observed 0.3—10 keV flux for an APEC spectrum with a temperature of 1 keV absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0_neg*FixedAPECECFO, so does not include uncertainties in the spectral modelling.
double
FixedAPECUnabsFlux
The unabsorbed 0.3—10 keV flux (in erg cm-2 s-1) derived from an APEC spectrum with a temperature of 1 keV absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0*FixedAPECECFU.
double
FixedAPECUnabsFlux_pos
The 1-σ positive error on the unabsorbed 0.3—10 keV flux for an APEC spectrum with a temperature of 1 keV absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0_pos*FixedAPECECFU, so does not include uncertainties in the spectral modelling.
double
FixedAPECUnabsFlux_neg
The 1-σ negative error on the unabsorbed 0.3—10 keV flux for an APEC spectrum with a temperature of 1 keV absorbed by the Galactic column (from the GalacticNH field). This is given by Rate_band0_neg*FixedAPECECFU, so does not include uncertainties in the spectral modelling.
double
InterpPowECFO
The counts-to-observed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from the hardness ratios of the source interpolated on a look-up table of power-law spectra.
double
InterpPowECFU
The counts-to-unabsorbed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from the hardness ratios of the source interpolated on a look-up table of power-law spectra.
double
InterpPowNH
The absorption column (in cm-2) of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of power-law spectra.
double
InterpPowNH_pos
The 1-σ positive error absorption column of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of power-law spectra. A value of -1 indicates that this error could not be constrained.
double
InterpPowNH_neg
The 1-σ negative error absorption column of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of power-law spectra. A value of +1 indicates that this error could not be constrained.
double
InterpPowGamma
The power-law photon index of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of power-law spectra.
double
InterpPowGamma_pos
The 1-σ positive error on the power-law photon index of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of power-law spectra. A value of -1 indicates that this error could not be constrained.
double
InterpPowGamma_neg
The 1-σ negative error on the power-law photon index of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of power-law spectra. A value of +1 indicates that this error could not be constrained.
double
InterpPowFlux
The observed 0.3—10 keV flux (in erg cm-2 s-1) based on the HR-interpolated power-law spectrum. This is given by Rate_band0*InterpPowECFO.
double
InterpPowFlux_pos
The 1-σ positive error on the observed 0.3—10 keV flux derived based on the HR-interpolated power-law spectrum. This is given by Rate_band0_pos*InterpPowECFO, so does not include uncertainties in the spectral modelling.
double
InterpPowFlux_neg
The 1-σ negative error on the observed 0.3—10 keV flux derived based on the HR-interpolated power-law spectrum. This is given by Rate_band0_neg*InterpPowECFO, so does not include uncertainties in the spectral modelling.
double
InterpPowUnabsFlux
The unabsorbed 0.3—10 keV flux (in erg cm-2 s-1) based on the HR-interpolated power-law spectrum. This is given by Rate_band0*InterpPowECFU.
double
InterpPowUnabsFlux_pos
The 1-σ positive error on the unabsorbed 0.3—10 keV flux derived based on the HR-interpolated power-law spectrum. This is given by Rate_band0_pos*InterpPowECFU, so does not include uncertainties in the spectral modelling.
double
InterpPowUnabsFlux_neg
The 1-σ negative error on the unabsorbed 0.3—10 keV flux derived based on the HR-interpolated power-law spectrum. This is given by Rate_band0_neg*InterpPowECFU, so does not include uncertainties in the spectral modelling.
double
InterpAPECECFO
The counts-to-observed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from the hardness ratios of the source interpolated on a look-up table of APEC spectra.
double
InterpAPECECFU
The counts-to-unabsorbed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from the hardness ratios of the source interpolated on a look-up table of APEC spectra.
double
InterpAPECNH
The absorption column (in cm-2) of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of APEC spectra.
double
InterpAPECNH_pos
The 1-σ positive error absorption column of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of APEC spectra. A value of -1 indicates that this error could not be constrained.
double
InterpAPECNH_neg
The 1-σ negative error absorption column of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of APEC spectra. A value of +1 indicates that this error could not be constrained.
double
InterpAPECkT
The APEC plasma temperature (in keV) of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of APEC spectra.
double
InterpAPECkT_pos
The 1-σ positive error on the APEC plasma temperature of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of APEC spectra. A value of -1 indicates that this error could not be constrained.
double
InterpAPECkT_neg
The 1-σ negative error on the APEC plasma temperature of the spectrum of the source derived from the hardness ratios of the source interpolated on a look-up table of APEC spectra. A value of +1 indicates that this error could not be constrained.
double
InterpAPECFlux
The observed 0.3—10 keV flux (in erg cm-2 s-1) based on the HR-interpolated APEC spectrum. This is given by Rate_band0*InterpAPECECFO.
double
InterpAPECFlux_pos
The 1-σ positive error on the observed 0.3—10 keV flux derived based on the HR-interpolated APEC spectrum. This is given by Rate_band0_pos*InterpAPECECFO, so does not include uncertainties in the spectral modelling.
double
InterpAPECFlux_neg
The 1-σ negative error on the observed 0.3—10 keV flux derived based on the HR-interpolated APEC spectrum. This is given by Rate_band0_neg*InterpAPECECFO, so does not include uncertainties in the spectral modelling.
double
InterpAPECUnabsFlux
The unabsorbed 0.3—10 keV flux (in erg cm-2 s-1) based on the HR-interpolated APEC spectrum. This is given by Rate_band0*InterpAPECECFU.
double
InterpAPECUnabsFlux_pos
The 1-σ positive error on the unabsorbed 0.3—10 keV flux derived based on the HR-interpolated APEC spectrum. This is given by Rate_band0_pos*InterpAPECECFU, so does not include uncertainties in the spectral modelling.
double
InterpAPECUnabsFlux_neg
The 1-σ negative error on the unabsorbed 0.3—10 keV flux derived based on the HR-interpolated APEC spectrum. This is given by Rate_band0_neg*InterpAPECECFU, so does not include uncertainties in the spectral modelling.
double
P_pow
If the (HR1,HR2) values of the source lie inside the range allowed by the simple power-law spectrum, this field is 1. Otherwise it is the probability of obtaining the measured hardness ratios and errors if the true spectrum is that which gives (HR1,HR2) closest to the sources values.
double
P_APEC
If the (HR1,HR2) values of the source lie inside the range allowed by the simple APEC spectrum, this field is 1. Otherwise it is the probability of obtaining the measured hardness ratios and errors if the true spectrum is that which gives (HR1,HR2) closest to the sources values.
double
FittedPowECFO
The counts-to-observed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from an automated power-law spectral fit to an automatically-extracted spectrum of the source.
double
FittedPowECFU
The counts-to-unabsorbed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from an automated power-law spectral fit to an automatically-extracted spectrum of the source.
double
FittedPowNH
The absorption column (in cm-2) of the spectrum of the source from an automated power-law spectral fit to an automatically-extracted spectrum of the source.
double
FittedPowNH_pos
The 1-σ positive error absorption column of the spectrum of the source from an automated power-law spectral fit to an automatically-extracted spectrum of the source.
double
FittedPowNH_neg
The 1-σ negative error absorption column of the spectrum of the source from an automated power-law spectral fit to an automatically-extracted spectrum of the source.
double
FittedPowGamma
The power-law photon index of the spectrum of the source from an automated power-law spectral fit to an automatically-extracted spectrum of the source.
double
FittedPowGamma_pos
The 1-σ positive error on the power-law photon index of the spectrum of the source from an automated power-law spectral fit to an automatically-extracted spectrum of the source.
double
FittedPowGamma_neg
The 1-σ negative error on the power-law photon index of the spectrum of the source from an automated power-law spectral fit to an automatically-extracted spectrum of the source.
double
FittedPowFlux
The observed 0.3—10 keV flux (in erg cm-2 s-1) derived from an automated power-law spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0*FittedPowECFO.
double
FittedPowFlux_pos
The 1-σ positive error on the observed 0.3—10 keV flux derived from an automated power-law spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0_pos*FittedPowECFO, so does not include uncertainties in the spectral modelling.
double
FittedPowFlux_neg
The 1-σ negative error on the observed 0.3—10 keV flux derived from an automated power-law spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0_ne*FittedPowECFO, so does not include uncertainties in the spectral modelling.
double
FittedPowUnabsFlux
The unabsorbed 0.3—10 keV flux (in erg cm-2 s-1) derived from an automated power-law spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0*FittedPowECFO.
double
FittedPowUnabsFlux_pos
The 1-σ positive error on the unabsorbed 0.3—10 keV flux derived from an automated power-law spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0_pos*FittedPowECFU, so does not include uncertainties in the spectral modelling.
double
FittedPowUnabsFlux_neg
The 1-σ negative error on the unabsorbed 0.3—10 keV flux derived from an automated power-law spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0_neg*FittedPowECFU, so does not include uncertainties in the spectral modelling.
double
FittedPowCstat
The Cstatistic from the power-law spectral fit.
double
FittedPowDOF
The number of degrees of freedom in the power-law spectral fit.
short
FittedPowReducedChi2
double
FittedAPECECFO
The counts-to-observed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1) derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source.
double
FittedAPECECFU
The counts-to-unabsorbed-flux (0.3—10 keV) conversion factor (in erg cm-2 ct-1), derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source.
double
FittedAPECNH
The absorption column (in cm-2) of the spectrum of the source derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source.
double
FittedAPECNH_pos
The 1-σ positive error absorption column of the spectrum of the source derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source.
double
FittedAPECNH_neg
The 1-σ negative error absorption column of the spectrum of the source derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source.
double
FittedAPECkT
The APEC plasma temperature (in keV) of the spectrum of the source derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source.
double
FittedAPECkT_pos
The 1-σ positive error on the APEC plasma temperature of the spectrum of the source derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source.
double
FittedAPECkT_neg
The 1-σ negative error on the APEC plasma temperature of the spectrum of the source derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source.
double
FittedAPECFlux
The observed 0.3—10 keV flux (in erg cm-2 s-1) derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0*FittedAPECECFO.
double
FittedAPECFlux_pos
The 1-σ positive error on the observed 0.3—10 keV flux derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0_pos*FittedAPECECFO, so does not include uncertainties in the spectral modelling.
double
FittedAPECFlux_neg
The 1-σ negative error on the observed 0.3—10 keV flux derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0_ne*FittedAPECECFO, so does not include uncertainties in the spectral modelling.
double
FittedAPECUnabsFlux
The unabsorbed 0.3—10 keV flux (in erg cm-2 s-1) derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0*FittedAPECECFO.
double
FittedAPECUnabsFlux_pos
The 1-σ positive error on the unabsorbed 0.3—10 keV flux derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0_pos*FittedAPECECFU, so does not include uncertainties in the spectral modelling.
double
FittedAPECUnabsFlux_neg
The 1-σ negative error on the unabsorbed 0.3—10 keV flux derived from an automated APEC spectral fit to an automatically-extracted spectrum of the source. This is given by Rate_band0_neg*FittedAPECECFU, so does not include uncertainties in the spectral modelling.
double
FittedAPECCstat
The Cstatistic from the APEC spectral fit.
double
FittedAPECDOF
The number of degrees of freedom in the APEC spectral fit.
short
FittedAPECReducedChi2
double
HasSpec
Whether there is (1) or is not (0) an automatically-built spectrum for this source.
short
NumExternalMatches
short
NumExternalMatches_slim
short
MatchInROSHRI
Whether the object does (1) or does not (0) match an object in the Rosat HRI catalogue.
short
MatchIn2RXS
Whether the object does (1) or does not (0) match an object in the 2RXS catalogue.
short
MatchIn3XMMDR8
Whether the object does (1) or does not (0) match an object in the 3XMM-DR8 catalogue.
short
MatchIn3XMM_Stack
short
MatchInXMMSL2
Whether the object does (1) or does not (0) match an object in the XMMSL2 catalogue.
short
MatchInSwiftFT
Whether the object does (1) or does not (0) match an object in the SwiftFT catalogue.
short
MatchIn1SWXRT
Whether the object does (1) or does not (0) match an object in the 1SWXRT catalogue.
short
MatchInXRTGRB
Whether the object does (1) or does not (0) match a catalogued XRT position of a Gamma Ray Burst.
short
MatchInSDSSQSO
Whether the object does (1) or does not (0) match an object in the SDSS QSO DR14 catalogue.
short
MatchIn2MASS
Whether the object does (1) or does not (0) match a 2MASS source.
short
MatchInUSNOB1
Whether the object does (1) or does not (0) match a USNO-B1 source.
short
MatchIn2CSC
Whether the object does (1) or does not (0) match an object in the 2CSC (Chandra) catalogue.
short
MatchIn1SXPS
Whether the object does (1) or does not (0) match an object in the 1SXPS catalogue.
short
MatchInALLWISE
Whether the object does (1) or does not (0) match an object in the ALLWISE catalogue.
short
catalogues.mv_cat2whsp_fdw
cat2whsp_oid
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
recno
Record number assigned by the VizieR team. Should Not be used for identification.
meta.record
int
"2whspj"
Name of the object (HHMMSS.s+DDMMSS)
meta.id;meta.main
char
u_2whspj
[*] Uncertainty flag on 2WHSPJ
meta.code.error
char
"5bzcat"
5BZCat source
meta.id;meta.dataset
char
l_lognupeak
Limit flag on lognupeak (1)
meta.code.error
char
ra
Position from name (right ascension part)
deg
pos.eq.ra;meta.main
double
primary
dec
Position from name (declination part)
deg
pos.eq.dec;meta.main
double
primary
u_lognupeak
[*] Uncertainty flag on lognupeak
meta.code.error
char
l_lognufnu
Limit flag on lognufnu (1)
meta.code.error
char
lognupeak
Synchrotron peak
[Hz]
em.freq
double
primary
lognufnu
Synchrotron peak flux (log(erg/s/cm2))
[mW/m2]
phot.flux
double
primary
u_lognufnu
[*] Uncertainty flag on lognufnu
meta.code.error
char
l_z
Limit flag on z
meta.code.error;src.redshift
char
z
? Redshift
src.redshift
double
primary
u_z
[*] Uncertainty flag on z
meta.code.error;src.redshift
char
r_z
[bcdefg] Reference on z (2)
meta.ref;pos.frame
char
"fermi-lat"
Fermi gamma-ray detection (3)
meta.id
char
gamma
Fermi gamma-ray photon index
spect.index
double
e_gamma
Photon index error
stat.error
double
"2fhl"
2FHL source name (HHMM.m+DDd, J2000)
meta.id
char
fom
Figure of Merit
meta.bib.fig
double
catalogues.mv_chandra_csc211_fdw
chandra_csc211_oid
null
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
name
Source name in the format '2CXO Jhhmmss.s{+|-}ddmmss[X]'
meta.id;meta.main
char
primary
ra
Source position, ICRS right ascension
deg
pos.eq.ra;meta.main
double
primary
dec
Source position, ICRS declination
deg
pos.eq.dec;meta.main
double
primary
err_ellipse_r0
Major radius of the 95% confidence level position error ellipse
arcsec
double
primary
err_ellipse_r1
Minor radius of the 95% confidence level position error ellipse
arcsec
double
primary
err_ellipse_ang
Position angle (ref. local true north) of the major axis of the 95% confidence level error ellipse
deg
double
primary
gal_b
Source position, Galactic latitude (equinox J2000.0, epoch J2000.0)
deg
pos.galactic.lat
double
gal_l
Source position, Galactic longitude (equinox J2000.0, epoch J2000.0)
deg
pos.galactic.lon
double
extent_flag
Source is extended, or deconvolved source extent is inconsistent with a point source at the 90% confidence level in one or more observations and energy bands
boolean
primary
conf_flag
Source may be confused (source and/or background regions overlap in one or more contributing stacked observations)
boolean
primary
pileup_flag
ACIS pile-up fraction exceeds ~ 10% in all observations; source properties may be affected
boolean
var_flag
Source displays flux variability within one or more observations, or between observations, in one or more energy bands
boolean
primary
streak_src_flag
Source is located on an ACIS readout streak in all observations; source properties may be affected
boolean
primary
sat_src_flag
Source is saturated in all observations; source properties are unreliable
boolean
primary
man_add_flag
Source was manually added in the catalog via human review
boolean
man_inc_flag
Source was manually included in the catalog via human review (detection was rejected by automated criteria)
boolean
man_reg_flag
Source region parameters (dimensions, initial guess position input to the Maximum Likelihood Estimator fit) were manually modified via human review
boolean
man_match_flag
Source detections were manually matched between overlapping stacked observations via human review
boolean
man_pos_flag
Best fit source position was manually modified via human review
boolean
var_inter_hard_flag
Source hardness ratios are statistically inconsistent between two or more observations
boolean
primary
major_axis_b
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy band
arcsec
double
major_axis_h
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy band
arcsec
double
major_axis_m
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy band
arcsec
double
major_axis_s
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy band
arcsec
double
major_axis_u
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy band
arcsec
double
major_axis_w
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy band
arcsec
double
major_axis_lolim_b
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
arcsec
double
major_axis_lolim_h
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
arcsec
double
major_axis_lolim_m
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
arcsec
double
major_axis_lolim_s
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
arcsec
double
major_axis_lolim_u
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
arcsec
double
major_axis_lolim_w
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
arcsec
double
major_axis_hilim_b
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
arcsec
double
major_axis_hilim_h
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
arcsec
double
major_axis_hilim_m
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
arcsec
double
major_axis_hilim_s
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
arcsec
double
major_axis_hilim_u
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
arcsec
double
major_axis_hilim_w
1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
arcsec
double
minor_axis_b
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy band
arcsec
double
minor_axis_h
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy band
arcsec
double
minor_axis_m
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy band
arcsec
double
minor_axis_s
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy band
arcsec
double
minor_axis_u
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy band
arcsec
double
minor_axis_w
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy band
arcsec
double
minor_axis_lolim_b
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
arcsec
double
minor_axis_lolim_h
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
arcsec
double
minor_axis_lolim_m
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
arcsec
double
minor_axis_lolim_s
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
arcsec
double
minor_axis_lolim_u
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
arcsec
double
minor_axis_lolim_w
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
arcsec
double
minor_axis_hilim_b
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
arcsec
double
minor_axis_hilim_h
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
arcsec
double
minor_axis_hilim_m
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
arcsec
double
minor_axis_hilim_s
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
arcsec
double
minor_axis_hilim_u
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
arcsec
double
minor_axis_hilim_w
1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
arcsec
double
pos_angle_b
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy band
deg
double
pos_angle_h
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy band
deg
double
pos_angle_m
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy band
deg
double
pos_angle_s
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy band
deg
double
pos_angle_u
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy band
deg
double
pos_angle_w
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy band
deg
double
pos_angle_lolim_b
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
deg
double
pos_angle_lolim_h
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
deg
double
pos_angle_lolim_m
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
deg
double
pos_angle_lolim_s
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
deg
double
pos_angle_lolim_u
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
deg
double
pos_angle_lolim_w
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
deg
double
pos_angle_hilim_b
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
deg
double
pos_angle_hilim_h
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
deg
double
pos_angle_hilim_m
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
deg
double
pos_angle_hilim_s
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
deg
double
pos_angle_hilim_u
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
deg
double
pos_angle_hilim_w
Position angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
deg
double
src_area_b
Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS broad (0.5-7.0 keV) energy band
arcsec**2
double
src_area_h
Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS hard (2.0-7.0 keV) energy band
arcsec**2
double
src_area_m
Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS medium (1.2-2.0 keV) energy band
arcsec**2
double
src_area_s
Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS soft (0.5-1.2 keV) energy band
arcsec**2
double
src_area_u
Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS ultrasoft (0.2-0.5 keV) energy band
arcsec**2
double
src_area_w
Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; HRC wide (~0.1-10.0 keV) energy band
arcsec**2
double
phot_nsrcs
Number of sources fit simultaneously to compute aperture photometry quantities
int
photflux_aper_b
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
photon/s/cm**2
double
photflux_aper_h
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
photon/s/cm**2
double
photflux_aper_m
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
photon/s/cm**2
double
photflux_aper_s
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
photon/s/cm**2
double
photflux_aper_u
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
photon/s/cm**2
double
photflux_aper_w
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC w
photon/s/cm**2
double
photflux_aper_lolim_b
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
photon/s/cm**2
double
photflux_aper_lolim_h
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
photon/s/cm**2
double
photflux_aper_lolim_m
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
photon/s/cm**2
double
photflux_aper_lolim_s
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
photon/s/cm**2
double
photflux_aper_lolim_u
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
photon/s/cm**2
double
photflux_aper_lolim_w
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
photon/s/cm**2
double
photflux_aper_hilim_b
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
photon/s/cm**2
double
photflux_aper_hilim_h
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
photon/s/cm**2
double
photflux_aper_hilim_m
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
photon/s/cm**2
double
photflux_aper_hilim_s
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
photon/s/cm**2
double
photflux_aper_hilim_u
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
photon/s/cm**2
double
photflux_aper_hilim_w
Aperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
photon/s/cm**2
double
photflux_aper90_b
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS br
photon/s/cm**2
double
photflux_aper90_h
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS ha
photon/s/cm**2
double
photflux_aper90_m
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS me
photon/s/cm**2
double
photflux_aper90_s
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS so
photon/s/cm**2
double
photflux_aper90_u
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS ul
photon/s/cm**2
double
photflux_aper90_w
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC wid
photon/s/cm**2
double
photflux_aper90_lolim_b
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
photon/s/cm**2
double
photflux_aper90_lolim_h
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
photon/s/cm**2
double
photflux_aper90_lolim_m
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
photon/s/cm**2
double
photflux_aper90_lolim_s
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
photon/s/cm**2
double
photflux_aper90_lolim_u
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
photon/s/cm**2
double
photflux_aper90_lolim_w
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
photon/s/cm**2
double
photflux_aper90_hilim_b
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
photon/s/cm**2
double
photflux_aper90_hilim_h
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
photon/s/cm**2
double
photflux_aper90_hilim_m
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
photon/s/cm**2
double
photflux_aper90_hilim_s
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
photon/s/cm**2
double
photflux_aper90_hilim_u
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
photon/s/cm**2
double
photflux_aper90_hilim_w
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
photon/s/cm**2
double
flux_aper_b
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
erg/s/cm**2
double
primary
flux_aper_h
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
erg/s/cm**2
double
flux_aper_m
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
erg/s/cm**2
double
flux_aper_s
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
erg/s/cm**2
double
flux_aper_u
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS
erg/s/cm**2
double
flux_aper_w
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC w
erg/s/cm**2
double
primary
flux_aper_lolim_b
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
erg/s/cm**2
double
primary
flux_aper_lolim_h
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
erg/s/cm**2
double
flux_aper_lolim_m
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
erg/s/cm**2
double
flux_aper_lolim_s
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
erg/s/cm**2
double
flux_aper_lolim_u
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
erg/s/cm**2
double
flux_aper_lolim_w
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% l
erg/s/cm**2
double
primary
flux_aper_hilim_b
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
erg/s/cm**2
double
primary
flux_aper_hilim_h
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
erg/s/cm**2
double
flux_aper_hilim_m
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
erg/s/cm**2
double
flux_aper_hilim_s
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
erg/s/cm**2
double
flux_aper_hilim_u
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
erg/s/cm**2
double
flux_aper_hilim_w
Aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% u
erg/s/cm**2
double
primary
flux_aper90_b
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS br
erg/s/cm**2
double
flux_aper90_h
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS ha
erg/s/cm**2
double
flux_aper90_m
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS me
erg/s/cm**2
double
flux_aper90_s
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS so
erg/s/cm**2
double
flux_aper90_u
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS ul
erg/s/cm**2
double
flux_aper90_w
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC wid
erg/s/cm**2
double
flux_aper90_lolim_b
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
erg/s/cm**2
double
flux_aper90_lolim_h
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
erg/s/cm**2
double
flux_aper90_lolim_m
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
erg/s/cm**2
double
flux_aper90_lolim_s
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
erg/s/cm**2
double
flux_aper90_lolim_u
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
erg/s/cm**2
double
flux_aper90_lolim_w
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% low
erg/s/cm**2
double
flux_aper90_hilim_b
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
erg/s/cm**2
double
flux_aper90_hilim_h
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
erg/s/cm**2
double
flux_aper90_hilim_m
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
erg/s/cm**2
double
flux_aper90_hilim_s
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
erg/s/cm**2
double
flux_aper90_hilim_u
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
erg/s/cm**2
double
flux_aper90_hilim_w
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upp
erg/s/cm**2
double
photflux_aper_avg_b
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_h
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_m
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_s
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_u
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_w
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_lolim_b
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_lolim_h
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_lolim_m
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_lolim_s
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_lolim_u
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_lolim_w
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_hilim_b
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_hilim_h
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_hilim_m
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_hilim_s
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_hilim_u
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
photon/s/cm**2
double
photflux_aper_avg_hilim_w
Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_b
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_h
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_m
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_s
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_u
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_w
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_lolim_b
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_lolim_h
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_lolim_m
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_lolim_s
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_lolim_u
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_lolim_w
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_hilim_b
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_hilim_h
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_hilim_m
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_hilim_s
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_hilim_u
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
photon/s/cm**2
double
photflux_aper90_avg_hilim_w
Aperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
photon/s/cm**2
double
flux_aper_avg_b
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
primary
flux_aper_avg_h
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_aper_avg_m
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_aper_avg_s
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_aper_avg_u
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_aper_avg_w
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
primary
flux_aper_avg_lolim_b
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
primary
flux_aper_avg_lolim_h
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_aper_avg_lolim_m
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_aper_avg_lolim_s
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_aper_avg_lolim_u
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_aper_avg_lolim_w
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
primary
flux_aper_avg_hilim_b
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
primary
flux_aper_avg_hilim_h
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_aper_avg_hilim_m
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_aper_avg_hilim_s
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_aper_avg_hilim_u
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_aper_avg_hilim_w
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
primary
flux_aper90_avg_b
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_h
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_m
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_s
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_u
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_w
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_lolim_b
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_lolim_h
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_lolim_m
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_lolim_s
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_lolim_u
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_lolim_w
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_hilim_b
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_hilim_h
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_hilim_m
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_hilim_s
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_hilim_u
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_aper90_avg_hilim_w
Aperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_b
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_h
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_m
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_s
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_u
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_w
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_lolim_b
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_lolim_h
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_lolim_m
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_lolim_s
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_lolim_u
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_lolim_w
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_hilim_b
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_hilim_h
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_hilim_m
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_hilim_s
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_hilim_u
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper_hilim_w
Source region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_lolim_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_lolim_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_lolim_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_lolim_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_lolim_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_lolim_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_hilim_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_hilim_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_hilim_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_hilim_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_hilim_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_powlaw_aper90_hilim_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_b
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_h
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_m
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_s
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_bb_aper_u
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_bb_aper_w
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_lolim_b
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_lolim_h
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_lolim_m
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_lolim_s
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_bb_aper_lolim_u
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_bb_aper_lolim_w
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_hilim_b
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_hilim_h
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_hilim_m
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper_hilim_s
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_bb_aper_hilim_u
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_bb_aper_hilim_w
Source region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_lolim_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_lolim_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_lolim_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_lolim_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_lolim_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_lolim_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_hilim_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_hilim_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_hilim_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_hilim_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_hilim_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_bb_aper90_hilim_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_b
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_h
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_m
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_s
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_brems_aper_u
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_brems_aper_w
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_lolim_b
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_lolim_h
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_lolim_m
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_lolim_s
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_brems_aper_lolim_u
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_brems_aper_lolim_w
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_hilim_b
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_hilim_h
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_hilim_m
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper_hilim_s
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_brems_aper_hilim_u
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_brems_aper_hilim_w
Source region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_lolim_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_lolim_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_lolim_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_lolim_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_lolim_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_lolim_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_hilim_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_hilim_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_hilim_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_hilim_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_hilim_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_brems_aper90_hilim_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_b
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_h
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_m
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_s
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_apec_aper_u
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_apec_aper_w
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_lolim_b
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_lolim_h
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_lolim_m
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_lolim_s
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_apec_aper_lolim_u
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_apec_aper_lolim_w
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_hilim_b
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_hilim_h
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_hilim_m
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper_hilim_s
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_apec_aper_hilim_u
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_apec_aper_hilim_w
Source region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_lolim_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_lolim_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_lolim_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_lolim_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_lolim_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_lolim_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_hilim_b
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_hilim_h
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_hilim_m
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_hilim_s
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_hilim_u
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
erg/s/cm**2
double
flux_apec_aper90_hilim_w
PSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band
erg/s/cm**2
double
likelihood
Highest detection log likelihood across all stacked observations and energy bands
double
primary
likelihood_class
Highest detection likelihood classification across all stacked observations and energy bands
char
primary
significance
Highest flux significance (S/N) across all stacked observations and energy bands
double
primary
flux_powlaw
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum
erg/s/cm**2
double
flux_powlaw_lolim
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
erg/s/cm**2
double
flux_powlaw_hilim
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
erg/s/cm**2
double
powlaw_gamma
Photon index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum
double
powlaw_gamma_lolim
Photon index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
double
powlaw_gamma_hilim
Photon index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
double
powlaw_gamma_rhat
Photon index convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum
double
powlaw_nh
N_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum
10**20/cm**2
double
powlaw_nh_lolim
N_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
10**20/cm**2
double
powlaw_nh_hilim
N_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
10**20/cm**2
double
powlaw_nh_rhat
N_H column density convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum
double
powlaw_ampl
Amplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum
double
powlaw_ampl_lolim
Amplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
double
powlaw_ampl_hilim
Amplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)
double
powlaw_ampl_rhat
Amplitude convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum
double
powlaw_stat
chi-square statistic per degree of freedom of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum
double
flux_bb
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum
erg/s/cm**2
double
flux_bb_lolim
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
erg/s/cm**2
double
flux_bb_hilim
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
erg/s/cm**2
double
bb_kt
Temperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum
keV
double
bb_kt_lolim
Temperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
keV
double
bb_kt_hilim
Temperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
keV
double
bb_kt_rhat
Temperature (kT) convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum
double
bb_nh
N_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum
10**20/cm**2
double
bb_nh_lolim
N_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
10**20/cm**2
double
bb_nh_hilim
N_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
10**20/cm**2
double
bb_nh_rhat
N_H column density convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum
double
bb_ampl
Amplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum
double
bb_ampl_lolim
Amplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
double
bb_ampl_hilim
Amplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)
double
bb_ampl_rhat
Amplitude convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum
double
bb_stat
chi-square statistic per degree of freedom of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum
double
flux_brems
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum
erg/s/cm**2
double
flux_brems_lolim
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
erg/s/cm**2
double
flux_brems_hilim
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
erg/s/cm**2
double
brems_kt
Temperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum
keV
double
brems_kt_lolim
Temperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
keV
double
brems_kt_hilim
Temperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
keV
double
brems_kt_rhat
Temperature (kT) convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum
double
brems_nh
N_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum
10**20/cm**2
double
brems_nh_lolim
N_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
10**20/cm**2
double
brems_nh_hilim
N_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
10**20/cm**2
double
brems_nh_rhat
N_H column density convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum
double
brems_norm
Amplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum
double
brems_norm_lolim
Amplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
double
brems_norm_hilim
Amplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)
double
brems_norm_rhat
Amplitude convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum
double
brems_stat
chi-square statistic per degree of freedom of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum
double
flux_apec
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
erg/s/cm**2
double
flux_apec_lolim
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
erg/s/cm**2
double
flux_apec_hilim
Net integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
erg/s/cm**2
double
apec_kt
Temperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
keV
double
apec_kt_lolim
Temperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
keV
double
apec_kt_hilim
Temperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
keV
double
apec_kt_rhat
Temperature (kT) convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
apec_abund
Abundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
apec_abund_lolim
Abundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
double
apec_abund_hilim
Abundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
double
apec_abund_rhat
Abundance convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
apec_z
Redshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
apec_z_lolim
Redshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
double
apec_z_hilim
Redshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
double
apec_z_rhat
Redshift convergence criterion Redshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
apec_nh
N_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
10**20/cm**2
double
apec_nh_lolim
N_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
10**20/cm**2
double
apec_nh_hilim
N_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)
10**20/cm**2
double
apec_nh_rhat
N_H column density convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
apec_norm
Amplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
apec_norm_lolim
Amplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)
double
apec_norm_hilim
Amplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)
double
apec_norm_rhat
Amplitude convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
apec_stat
chi-square statistic per degree of freedom of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum
double
nh_gal
Galactic N_H column density in direction of source
10**20/cm**2
double
hard_hm
ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio
double
primary
hard_hm_lolim
ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% lower confidence limit)
double
primary
hard_hm_hilim
ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% upper confidence limit)
double
primary
var_inter_hard_prob_hm
Inter-observation ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio variability probability
double
primary
var_inter_hard_sigma_hm
Inter-observation ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio variability standard deviation
double
hard_hs
ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio
double
hard_hs_lolim
ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)
double
hard_hs_hilim
ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)
double
var_inter_hard_prob_hs
Inter-observation ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio variability probability
double
var_inter_hard_sigma_hs
Inter-observation ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio variability standard deviation
double
hard_ms
ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio
double
primary
hard_ms_lolim
ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)
double
primary
hard_ms_hilim
ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)
double
primary
var_inter_hard_prob_ms
Inter-observation ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio variability probability
double
primary
var_inter_hard_sigma_ms
Inter-observation ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio variability standard deviation
double
ks_intra_prob_b
Intra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy band
double
ks_intra_prob_h
Intra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy band
double
ks_intra_prob_m
Intra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy band
double
ks_intra_prob_s
Intra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy band
double
ks_intra_prob_u
Intra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy band
double
ks_intra_prob_w
Intra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy band
double
kp_intra_prob_b
Intra-observation Kuiper's test variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy band
double
kp_intra_prob_h
Intra-observation Kuiper's test variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy band
double
kp_intra_prob_m
Intra-observation Kuiper's test variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy band
double
kp_intra_prob_s
Intra-observation Kuiper's test variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy band
double
kp_intra_prob_u
Intra-observation Kuiper's test variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy band
double
kp_intra_prob_w
Intra-observation Kuiper's test variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy band
double
var_intra_prob_b
Intra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy band
double
var_intra_prob_h
Intra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy band
double
var_intra_prob_m
Intra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy band
double
var_intra_prob_s
Intra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy band
double
var_intra_prob_u
Intra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy band
double
var_intra_prob_w
Intra-observation Gregory-Loredo variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy band
double
var_intra_index_b
Intra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS broad (0.5-7.0 keV) energy band
int
primary
var_intra_index_h
Intra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS hard (2.0-7.0 keV) energy band
int
var_intra_index_m
Intra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS medium (1.2-2.0 keV) energy band
int
var_intra_index_s
Intra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS soft (0.5-1.2 keV) energy band
int
var_intra_index_u
Intra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy band
int
var_intra_index_w
Intra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); HRC wide (~0.1-10.0 keV) energy band
int
primary
var_inter_prob_b
Inter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS broad (0.5-7.0 keV) energy band
double
var_inter_prob_h
Inter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS hard (2.0-7.0 keV) energy band
double
var_inter_prob_m
Inter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS medium (1.2-2.0 keV) energy band
double
var_inter_prob_s
Inter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS soft (0.5-1.2 keV) energy band
double
var_inter_prob_u
Inter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS ultrasoft (0.2-0.5 keV) energy band
double
var_inter_prob_w
Inter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; HRC wide (~0.1-10.0 keV) energy band
double
var_inter_index_b
Inter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS broad (0.5-7.0 keV) energy band
int
primary
var_inter_index_h
Inter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS hard (2.0-7.0 keV) energy band
int
var_inter_index_m
Inter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS medium (1.2-2.0 keV) energy band
int
var_inter_index_s
Inter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS soft (0.5-1.2 keV) energy band
int
var_inter_index_u
Inter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS ultrasoft (0.2-0.5 keV) energy band
int
var_inter_index_w
Inter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; HRC wide (~0.1-10.0 keV) energy band
int
primary
var_inter_sigma_b
Inter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS broad (0.5-7.0 keV) energy band
photon/s/cm**2
double
var_inter_sigma_h
Inter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS hard (2.0-7.0 keV) energy band
photon/s/cm**2
double
var_inter_sigma_m
Inter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS medium (1.2-2.0 keV) energy band
photon/s/cm**2
double
var_inter_sigma_s
Inter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS soft (0.5-1.2 keV) energy band
photon/s/cm**2
double
var_inter_sigma_u
Inter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS ultrasoft (0.2-0.5 keV) energy band
photon/s/cm**2
double
var_inter_sigma_w
Inter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; HRC wide (~0.1-10.0 keV) energy band
photon/s/cm**2
double
dither_warning_flag
Highest statistically significant peak in the power spectrum of the source region count rate occurs at the dither frequency or at a beat frequency of the dither frequency in one or more observations
boolean
acis_num
Total number of ACIS imaging observations contributing to the Master Sources Table record of the source
int
acis_hetg_num
Total number of ACIS/HETG observations contributing to the Master Sources Table record of the source
int
acis_letg_num
Total number of ACIS/LETG observations contributing to the Master Sources Table record of the source
int
acis_time
Total exposure time (seconds of good time) for all ACIS imaging observations contributing to the Master Sources Table record of the source
s
double
primary
acis_hetg_time
Total exposure time (seconds of good time) for all ACIS/HETG observations contributing to the Master Sources Table record of the source
s
double
acis_letg_time
Total exposure time (seconds of good time) for all ACIS/LETG observations contributing to the Master Sources Table record of the source
s
double
hrc_num
Total number of HRC imaging observations contributing to the Master Sources Table record of the source
int
hrc_hetg_num
Total number of HRC/HETG observations contributing to the Master Sources Table record of the source
int
hrc_letg_num
Total number of HRC/LETG observations contributing to the Master Sources Table record of the source
int
hrc_time
Total exposure time (seconds of good time) for all HRC imaging observations contributing to the Master Sources Table record of the source
s
double
primary
hrc_hetg_time
Total exposure time (seconds of good time) for all HRC/HETG observations contributing to the Master Sources Table record of the source
s
double
hrc_letg_time
Total exposure time (seconds of good time) for all HRC/LETG observations contributing to the Master Sources Table record of the source
s
double
catalogues.mv_efeds_c001_hard_fdw
efeds_c001_hard_oid
null
meta.oid
int
name
Source name
meta.id;meta.main;src
char
primary
npix
Healpix pixel of the center of the observation for nside 256
long
ra_corr
Corrected RA (ICRS)
deg
pos.eq.ra;meta.main
double
primary
dec_corr
Corrected Dec (ICRS)
deg
pos.eq.dec;meta.main
double
primary
id_src
Source ID
meta.id;src
int
id_main
Source ID in the single-band detected, eFEDS main catalog
meta.id
int
ml_flux_b1
Source flux converted from count rate; 0.2-0.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
primary
ml_flux_err_b1
1 sigma flux error; 0.2-0.5 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
primary
ra
Uncorrected RA (ICRS)
deg
pos.eq.ra;stat.uncalib
double
dec
Uncorrected Dec (ICRS)
deg
pos.eq.dec;stat.uncalib
double
ml_flux_b2
Source flux converted from count rate; 0.5-1 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
primary
ml_flux_err_b2
1 sigma flux error; 0.5-1 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
primary
radec_err
Combined positional uncertainty, uncorrected
arcsec
stat.error;pos;stat.uncalib
double
ml_flux_b3
Source flux converted from count rate; 1-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
primary
ml_flux_err_b3
1 sigma flux error; 1-2 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
primary
ml_flux_b4
Source flux converted from count rate; 2-4.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
primary
radec_err_corr
Combined positional uncertainty, corrected
arcsec
stat.error;pos
double
ext
Source extent
arcsec
phys.angSize;em.X-ray.soft
double
ml_flux_err_b4
1 sigma flux error; 2-4.5 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.medium
double
primary
ext_err
Extent error
arcsec
stat.error;phys.angSize;em.X-ray
double
ext_like
Extent likelihood
stat.likelihood
double
det_like_0
Detection likelihood measured by PSF-fitting
stat.likelihood
double
ml_rate_0
Source count rate
counts/s
arith.rate;phot.count
double
ml_rate_err_0
1 sigma count rate error
counts/s
stat.error;phot.count
double
ml_cts_0
Source net counts, combining 3 bands
counts
phot.count
double
ml_cts_err_0
1 sigma counts error
counts
stat.error;phot.count
double
ml_flux_0
Source flux
erg.s-1.cm-2
phot.flux
double
ml_flux_err_0
1 sigma flux error
erg.s-1.cm-2
stat.error;phot.flux
double
ml_bkg_0
Background flux at the source position
counts/arcmin^2
instr.background
double
inarea90
meta.code;pos
boolean
det_like_1
Detection likelihood measured by PSF-fitting
stat.likelihood
double
det_like_2
Detection likelihood measured by PSF-fitting
stat.likelihood
double
det_like_3
Detection likelihood measured by PSF-fitting
stat.likelihood
double
ml_rate_1
Source count rate measured by PSF-fitting
counts/s
arith.rate;phot.count
double
ml_rate_2
Source count rate measured by PSF-fitting
counts/s
arith.rate;phot.count
double
ml_rate_3
Source count rate measured by PSF-fitting
counts/s
arith.rate;phot.count
double
ml_rate_err_1
1 sigma count rate error
counts/s
stat.error;phot.count
double
ml_rate_err_2
1 sigma count rate error
counts/s
stat.error;phot.count
double
ml_rate_err_3
1 sigma count rate error
counts/s
stat.error;phot.count
double
ml_cts_1
Source net counts measured from count rate
counts
phot.count
double
ml_cts_2
Source net counts measured from count rate
counts
phot.count
double
ml_cts_3
Source net counts measured from count rate
counts
phot.count
double
ml_cts_err_1
1 sigma counts error
counts
stat.error;phot.count
double
ml_cts_err_2
1 sigma counts error
counts
stat.error;phot.count
double
ml_cts_err_3
1 sigma counts error
counts
stat.error;phot.count
double
ml_flux_1
Source flux converted from count rate
erg.s-1.cm-2
phot.flux
double
ml_flux_2
Source flux converted from count rate
erg.s-1.cm-2
phot.flux
double
ml_flux_3
Source flux converted from count rate
erg.s-1.cm-2
phot.flux
double
ml_flux_err_1
1 sigma flux error
erg.s-1.cm-2
stat.error;phot.flux
double
ml_flux_err_2
1 sigma flux error
erg.s-1.cm-2
stat.error;phot.flux
double
ml_flux_err_3
1 sigma flux error
erg.s-1.cm-2
stat.error;phot.flux
double
ml_exp_1
Vignetted exposure value
seconds
time.duration;obs.exposure
double
ml_exp_2
Vignetted exposure value
seconds
time.duration;obs.exposure
double
ml_exp_3
Vignetted exposure value
seconds
time.duration;obs.exposure
double
ml_bkg_1
Background flux at the source position
counts/arcmin^2
instr.background
double
ml_bkg_2
Background flux at the source position
counts/arcmin^2
instr.background
double
ml_bkg_3
Background flux at the source position
counts/arcmin^2
instr.background
double
det_like_b1
Detection likelihood measured by forced PSF-fitting; 0.2-0.5 keV
stat.likelihood;em.X-ray.soft
double
det_like_b2
Detection likelihood measured by forced PSF-fitting; 0.5-1 keV
stat.likelihood;em.X-ray.soft
double
det_like_b3
Detection likelihood measured by forced PSF-fitting; 1-2 keV
stat.likelihood;em.X-ray.soft
double
det_like_b4
Detection likelihood measured by forced PSF-fitting; 2-4.5 keV
stat.likelihood;em.X-ray.medium
double
det_like_s
Detection likelihood measured by forced PSF-fitting; 0.5-2 keV
stat.likelihood;em.X-ray.soft
double
det_like_h
Detection likelihood measured by forced PSF-fitting; 2.3-5 keV
stat.likelihood;em.X-ray.medium
double
det_like_u
Detection likelihood measured by forced PSF-fitting; 5-8 keV
stat.likelihood;em.X-ray.medium
double
ml_rate_b1
Source count rate measured by forced PSF-fitting;.2-.5keV
counts/s
arith.rate;phot.count;em.X-ray.soft
double
ml_rate_b2
Source count rate measured by forced PSF-fitting;0.5-1keV
counts/s
arith.rate;phot.count;em.X-ray.soft
double
ml_rate_b3
Source count rate measured by forced PSF-fitting; 1-2 keV
counts/s
arith.rate;phot.count;em.X-ray.soft
double
ml_rate_b4
Source count rate measured by forced PSF-fitting;2-4.5keV
counts/s
arith.rate;phot.count;em.X-ray.medium
double
ml_rate_s
Source count rate measured by forced PSF-fitting;0.5-2keV
counts/s
arith.rate;phot.count;em.X-ray.soft
double
ml_rate_h
Source count rate measured by forced PSF-fitting;2.3-5keV
counts/s
arith.rate;phot.count;em.X-ray.medium
double
ml_rate_u
Source count rate measured by forced PSF-fitting; 5-8 keV
counts/s
arith.rate;phot.count;em.X-ray.medium
double
ml_rate_err_b1
1 sigma count rate error; 0.2-0.5 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_err_b2
1 sigma count rate error; 0.5-1 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_err_b3
1 sigma count rate error; 1-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_err_b4
1 sigma count rate error; 2-4.5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_err_s
1 sigma count rate error; 0.5-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_err_h
1 sigma count rate error; 2.3-5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_err_u
1 sigma count rate error; 5-8 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_lowerr_b1
1 sigma lower error of count rate;0.2-0.5 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_lowerr_b2
1 sigma lower error of count rate;0.5-1 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_lowerr_b3
1 sigma lower error of count rate;1-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_lowerr_b4
1 sigma lower error of count rate;2-4.5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_lowerr_s
1 sigma lower error of count rate;0.5-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_lowerr_h
1 sigma lower error of count rate;2.3-5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_lowerr_u
1 sigma lower error of count rate;5-8 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_uperr_b1
1 sigma upper error of count rate;0.2-0.5 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_uperr_b2
1 sigma upper error of count rate;0.5-1 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_uperr_b3
1 sigma upper error of count rate;1-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_uperr_b4
1 sigma upper error of count rate;2-4.5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_uperr_s
1 sigma upper error of count rate;0.5-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_uperr_h
1 sigma upper error of count rate;2.3-5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_uperr_u
1 sigma upper error of count rate;5-8 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_cts_b1
Source net counts measured from count rate; 0.2-0.5 keV
counts
phot.count;em.X-ray.soft
double
ml_cts_b2
Source net counts measured from count rate; 0.5-1 keV
counts
phot.count;em.X-ray.soft
double
ml_cts_b3
Source net counts measured from count rate; 1-2 keV
counts
phot.count;em.X-ray.soft
double
ml_cts_b4
Source net counts measured from count rate; 2-4.5 keV
counts
phot.count;em.X-ray.medium
double
ml_cts_s
Source net counts measured from count rate; 0.5-2 keV
counts
phot.count;em.X-ray.soft
double
ml_cts_h
Source net counts measured from count rate; 2.3-5 keV
counts
phot.count;em.X-ray.medium
double
ml_cts_u
Source net counts measured from count rate; 5-8 keV
counts
phot.count;em.X-ray.medium
double
ml_cts_err_b1
1 sigma counts error; 0.2-0.5 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_err_b2
1 sigma counts error; 0.5-1 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_err_b3
1 sigma counts error; 1-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_err_b4
1 sigma counts error; 2-4.5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_err_s
1 sigma counts error; 0.5-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_err_h
1 sigma counts error; 2.3-5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_err_u
1 sigma counts error; 5-8 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_lowerr_b1
1 sigma lower error of counts;0.2-0.5 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_lowerr_b2
1 sigma lower error of counts;0.5-1 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_lowerr_b3
1 sigma lower error of counts;1-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_lowerr_b4
1 sigma lower error of counts;2-4.5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_lowerr_s
1 sigma lower error of counts;0.5-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_lowerr_h
1 sigma lower error of counts;2.3-5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_lowerr_u
1 sigma lower error of counts;5-8 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_uperr_b1
1 sigma upper error of counts;0.2-0.5 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_uperr_b2
1 sigma upper error of counts;0.5-1 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_uperr_b3
1 sigma upper error of counts;1-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_uperr_b4
1 sigma upper error of counts;2-4.5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_uperr_s
1 sigma upper error of counts;0.5-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_uperr_h
1 sigma upper error of counts;2.3-5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_uperr_u
1 sigma upper error of counts;5-8 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_flux_s
Source flux converted from count rate; 0.5-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_h
Source flux converted from count rate; 2.3-5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_u
Source flux converted from count rate; 5-8 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_err_s
1 sigma flux error; 0.5-2 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
ml_flux_err_h
1 sigma flux error; 2.3-5 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.medium
double
ml_flux_err_u
1 sigma flux error; 5-8 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.medium
double
ml_flux_lowerr_b1
1 sigma lower error of flux;0.2-0.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_lowerr_b2
1 sigma lower error of flux;0.5-1 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_lowerr_b3
1 sigma lower error of flux;1-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_lowerr_b4
1 sigma lower error of flux;2-4.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_lowerr_s
1 sigma lower error of flux;0.5-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_lowerr_h
1 sigma lower error of flux;2.3-5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_lowerr_u
1 sigma lower error of flux;5-8 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_uperr_b1
1 sigma upper error of flux;0.2-0.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_uperr_b2
1 sigma upper error of flux;0.5-1 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_uperr_b3
1 sigma upper error of flux;1-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_uperr_b4
1 sigma upper error of flux;2-4.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_uperr_s
1 sigma upper error of flux;0.5-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_uperr_h
1 sigma upper error of flux;2.3-5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_uperr_u
1 sigma upper error of flux;5-8 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_exp_b1
Vignetted exposure value; 0.2-0.5 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ml_exp_b2
Vignetted exposure value; 0.5-1 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ml_exp_b3
Vignetted exposure value; 1-2 keV
seconds
uctime.duration;obs.exposure;em.X-ray.soft
double
ml_exp_b4
Vignetted exposure value; 2-4.5 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ml_exp_s
Vignetted exposure value; 0.5-2 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ml_exp_h
Vignetted exposure value; 2.3-5 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ml_exp_u
Vignetted exposure value; 5-8 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ml_bkg_b1
Background flux at the source position; 0.2-0.5keV
counts/arcmin^2
instr.background;em.X-ray.soft
double
ml_bkg_b2
Background flux at the source position; 0.5-1 keV
counts/arcmin^2
instr.background;em.X-ray.soft
double
ml_bkg_b3
Background flux at the source position; 1-2 keV
counts/arcmin^2
instr.background;em.X-ray.soft
double
ml_bkg_b4
Background flux at the source position; 2-4.5 keV
counts/arcmin^2
instr.background;em.X-ray.medium
double
ml_bkg_s
Background flux at the source position; 0.5-2 keV
counts/arcmin^2
instr.background;em.X-ray.soft
double
ml_bkg_h
Background flux at the source position; 2.3-5 keV
counts/arcmin^2
instr.background;em.X-ray.medium
double
ml_bkg_u
Background flux at the source position; 5-8 keV
counts/arcmin^2
instr.background;em.X-ray.medium
double
ape_cts_b1
Total counts extracted in the aperture; 0.2-0.5 keV
counts
phot.count;em.X-ray.soft
int
ape_cts_b2
Total counts extracted in the aperture; 0.5-1 keV
counts
phot.count;em.X-ray.soft
int
ape_cts_b3
Total counts extracted in the aperture; 1-2 keV
counts
phot.count;em.X-ray.soft
int
ape_cts_b4
Total counts extracted in the aperture; 2-4.5 keV
counts
phot.count;em.X-ray.medium
int
ape_cts_s
Total counts extracted in the aperture; 0.5-2 keV
counts
phot.count;em.X-ray.soft
int
ape_cts_h
Total counts extracted in the aperture; 2.3-5 keV
counts
phot.count;em.X-ray.medium
int
ape_cts_u
Total counts extracted in the aperture; 5-8 keV
counts
phot.count;em.X-ray.medium
int
ape_exp_b1
Vignetted exposure value; 0.2-0.5 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ape_exp_b2
Vignetted exposure value; 0.5-1 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ape_exp_b3
Vignetted exposure value; 1-2 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ape_exp_b4
Vignetted exposure value; 2-4.5 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ape_exp_s
Vignetted exposure value; 0.5-2 keV
seconds
uctime.duration;obs.exposured;em.X-ray.soft
double
ape_exp_h
Vignetted exposure value; 2.3-5 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ape_exp_u
Vignetted exposure value; 5-8 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ape_bkg_b1
Background counts in the aperture, excluding nearby
sources;.2-.5keV
counts
instr.background;em.X-ray.soft
double
ape_bkg_b2
Background counts in the aperture, excluding nearby
sources;0.5-1keV
counts
instr.background;em.X-ray.soft
double
ape_bkg_b3
Background counts in the aperture, excluding nearby sources; 1-2
keV
counts
instr.backgrounde;em.X-ray.soft
double
ape_bkg_b4
Background counts in the aperture, excluding nearby
sources;2-4.5keV
counts
instr.background;em.X-ray.medium
double
ape_bkg_s
Background counts in the aperture, excluding nearby
sources;0.5-2keV
counts
instr.background;em.X-ray.soft
double
ape_bkg_h
Background counts in the aperture, excluding nearby
sources;2.3-5keV
counts
instr.background;em.X-ray.medium
double
ape_bkg_u
Background counts in the aperture, excluding nearby sources; 5-8
keV
counts
instr.background;em.X-ray.medium
double
ape_radius_b1
Aperture radius; 0.2-0.5 keV
pixels
phys.angSize;instr.pixel;em.X-ray.soft
double
ape_radius_b2
Aperture radius; 0.5-1 keV
pixels
phys.angSize;instr.pixel;em.X-ray.soft
double
ape_radius_b3
Aperture radius; 1-2 keV
pixels
phys.angSize;instr.pixel;em.X-ray.soft
double
ape_radius_b4
Aperture radius; 2-4.5 keV
pixels
phys.angSize;instr.pixel;em.X-ray.medium
double
ape_radius_s
Aperture radius; 0.5-2 keV
pixels
phys.angSize;instr.pixel;em.X-ray.soft
double
ape_radius_h
Aperture radius; 2.3-5 keV
pixels
phys.angSize;instr.pixel;em.X-ray.medium
double
ape_radius_u
Aperture radius; 5-8 keV
pixels
phys.angSize;instr.pixel;em.X-ray.medium
double
ape_pois_b1
Poisson probability of being background fluctuation; 0.2-0.5 keV
stat.probability;em.X-ray.soft
double
ape_pois_b2
Poisson probability of being background fluctuation; 0.5-1 keV
stat.probability;em.X-ray.soft
double
ape_pois_b3
Poisson probability of being background fluctuation; 1-2 keV
stat.probability;em.X-ray.soft
double
ape_pois_b4
Poisson probability of being background fluctuation; 2-4.5 keV
stat.probability;em.X-ray.medium
double
ape_pois_s
Poisson probability of being background fluctuation; 0.5-2 keV
stat.probability;em.X-ray.soft
double
ape_pois_h
Poisson probability of being background fluctuation; 2.3-5 keV
stat.probability;em.X-ray.medium
double
ape_pois_u
Poisson probability of being background fluctuation; 5-8 keV
stat.probability;em.X-ray.medium
double
catalogues.mv_efeds_c001_main_fdw
efeds_c001_main_oid
null
meta.oid
int
name
Source name
meta.id;meta.main;src
char
primary
npix
Healpix pixel of the center of the observation for nside 256
long
ra_corr
Corrected RA (ICRS)
deg
pos.eq.ra;meta.main
double
primary
dec_corr
Corrected Dec (ICRS)
deg
pos.eq.dec;meta.main
double
primary
id_src
Source ID
meta.id;src
int
id_hard
Source ID in the eFEDS hard-band selected catalog
meta.id
int
ml_flux_b1
Source flux converted from count rate; 0.2-0.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
primary
ml_flux_err_b1
1 sigma flux error; 0.2-0.5 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
primary
ra
Uncorrected RA (ICRS)
deg
pos.eq.ra;stat.uncalib
double
dec
Uncorrected Dec (ICRS)
deg
pos.eq.dec;stat.uncalib
double
ml_flux_b2
Source flux converted from count rate; 0.5-1 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
primary
ml_flux_err_b2
1 sigma flux error; 0.5-1 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
primary
radec_err
Combined positional uncertainty, uncorrected
arcsec
stat.error;pos;stat.uncalib
double
ml_flux_b3
Source flux converted from count rate; 1-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
primary
ml_flux_err_b3
1 sigma flux error; 1-2 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
primary
ml_flux_b4
Source flux converted from count rate; 2-4.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
primary
radec_err_corr
Combined positional uncertainty, corrected
arcsec
stat.error;pos
double
ext
Source extent
arcsec
phys.angSize;em.X-ray.soft
double
ml_flux_err_b4
1 sigma flux error; 2-4.5 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.medium
double
primary
ext_err
Extent error
arcsec
stat.error;phys.angSize;em.X-ray
double
ext_like
Extent likelihood
stat.likelihood
double
det_like
Detection likelihood measured by PSF-fitting
stat.likelihood;em.X-ray
double
ml_rate
Source count rate measured by PSF-fitting
counts/s
arith.rate;phot.count;em.X-ray
double
ml_rate_err
1 sigma count rate error
counts/s
stat.error;phot.count;em.X-ray
double
ml_cts
Source net counts measured from count rate
counts
phot.count;em.X-ray
double
ml_cts_err
1 sigma counts error
counts
stat.error;phot.count
double
ml_flux
Source flux converted from count rate
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_err
1 sigma flux error
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray
double
ml_exp
Vignetted exposure value
seconds
time.duration;obs.exposure;em.X-ray
double
ml_bkg
Background at the source position
counts/arcmin^2
instr.background
double
inarea90
Whether in the 0.2-2.3keV exp>500s region, which comprises 90%
area
meta.code;pos
boolean
det_like_b1
Detection likelihood measured by forced PSF-fitting; 0.2-0.5 keV
stat.likelihood;em.X-ray.soft
double
det_like_b2
Detection likelihood measured by forced PSF-fitting; 0.5-1 keV
stat.likelihood;em.X-ray.soft
double
det_like_b3
Detection likelihood measured by forced PSF-fitting; 1-2 keV
stat.likelihood;em.X-ray.soft
double
det_like_b4
Detection likelihood measured by forced PSF-fitting; 2-4.5 keV
stat.likelihood;em.X-ray.medium
double
det_like_s
Detection likelihood measured by forced PSF-fitting; 0.5-2 keV
stat.likelihood;em.X-ray.soft
double
det_like_h
Detection likelihood measured by forced PSF-fitting; 2.3-5 keV
stat.likelihood;em.X-ray.medium
double
det_like_u
Detection likelihood measured by forced PSF-fitting; 5-8 keV
stat.likelihood;em.X-ray.medium
double
ml_rate_b1
Source count rate measured by forced PSF-fitting; .2-.5keV
counts/s
arith.rate;phot.count;em.X-ray.soft
double
ml_rate_b2
Source count rate measured by forced PSF-fitting; 0.5-1keV
counts/s
arith.rate;phot.count;em.X-ray.soft
double
ml_rate_b3
Source count rate measured by forced PSF-fitting; 1-2 keV
counts/s
arith.rate;phot.count;em.X-ray.soft
double
ml_rate_b4
Source count rate measured by forced PSF-fitting; 2-4.5keV
counts/s
arith.rate;phot.count;em.X-ray.medium
double
ml_rate_s
Source count rate measured by forced PSF-fitting; 0.5-2keV
counts/s
arith.rate;phot.count;em.X-ray.soft
double
ml_rate_h
Source count rate measured by forced PSF-fitting; 2.3-5keV
counts/s
arith.rate;phot.count;em.X-ray.medium
double
ml_rate_u
Source count rate measured by forced PSF-fitting; 5-8 keV
counts/s
arith.rate;phot.count;em.X-ray.medium
double
ml_rate_err_b1
1 sigma count rate error; 0.2-0.5 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_err_b2
1 sigma count rate error; 0.5-1 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_err_b3
1 sigma count rate error; 1-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_err_b4
1 sigma count rate error; 2-4.5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_err_s
1 sigma count rate error; 0.5-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_err_h
1 sigma count rate error; 2.3-5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_err_u
1 sigma count rate error; 5-8 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_lowerr_b1
1 sigma lower error of count rate;0.2-0.5 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_lowerr_b2
1 sigma lower error of count rate;0.5-1 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_lowerr_b3
1 sigma lower error of count rate;1-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_lowerr_b4
1 sigma lower error of count rate;2-4.5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_lowerr_s
1 sigma lower error of count rate;0.5-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_lowerr_h
1 sigma lower error of count rate;2.3-5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_lowerr_u
1 sigma lower error of count rate;5-8 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_uperr_b1
1 sigma upper error of count rate;0.2-0.5 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_uperr_b2
1 sigma upper error of count rate;0.5-1 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_uperr_b3
1 sigma upper error of count rate;1-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_uperr_b4
1 sigma upper error of count rate;2-4.5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_uperr_s
1 sigma upper error of count rate;0.5-2 keV
counts/s
stat.error;phot.count;em.X-ray.soft
double
ml_rate_uperr_h
1 sigma upper error of count rate;2.3-5 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_rate_uperr_u
1 sigma upper error of count rate;5-8 keV
counts/s
stat.error;phot.count;em.X-ray.medium
double
ml_cts_b1
Source net counts measured from count rate; 0.2-0.5 keV
counts
phot.count;em.X-ray.soft
double
ml_cts_b2
Source net counts measured from count rate; 0.5-1 keV
counts
phot.count;em.X-ray.soft
double
ml_cts_b3
Source net counts measured from count rate; 1-2 keV
counts
phot.count;em.X-ray.soft
double
ml_cts_b4
Source net counts measured from count rate; 2-4.5 keV
counts
phot.count;em.X-ray.medium
double
ml_cts_s
Source net counts measured from count rate; 0.5-2 keV
counts
phot.count;em.X-ray.soft
double
ml_cts_h
Source net counts measured from count rate; 2.3-5 keV
counts
phot.count;em.X-ray.medium
double
ml_cts_u
Source net counts measured from count rate; 5-8 keV
counts
phot.count;em.X-ray.medium
double
ml_cts_err_b1
1 sigma counts error; 0.2-0.5 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_err_b2
1 sigma counts error; 0.5-1 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_err_b3
1 sigma counts error; 1-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_err_b4
1 sigma counts error; 2-4.5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_err_s
1 sigma counts error; 0.5-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_err_h
1 sigma counts error; 2.3-5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_err_u
1 sigma counts error; 5-8 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_lowerr_b1
1 sigma lower error of counts;0.2-0.5 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_lowerr_b2
1 sigma lower error of counts;0.5-1 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_lowerr_b3
1 sigma lower error of counts;1-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_lowerr_b4
1 sigma lower error of counts;2-4.5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_lowerr_s
1 sigma lower error of counts;0.5-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_lowerr_h
1 sigma lower error of counts;2.3-5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_lowerr_u
1 sigma lower error of counts;5-8 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_uperr_b1
1 sigma upper error of counts;0.2-0.5 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_uperr_b2
1 sigma upper error of counts;0.5-1 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_uperr_b3
1 sigma upper error of counts;1-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_uperr_b4
1 sigma upper error of counts;2-4.5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_uperr_s
1 sigma upper error of counts;0.5-2 keV
counts
stat.error;phot.count;em.X-ray.soft
double
ml_cts_uperr_h
1 sigma upper error of counts;2.3-5 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_cts_uperr_u
1 sigma upper error of counts;5-8 keV
counts
stat.error;phot.count;em.X-ray.medium
double
ml_flux_s
Source flux converted from count rate; 0.5-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_h
Source flux converted from count rate; 2.3-5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_u
Source flux converted from count rate; 5-8 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_err_s
1 sigma flux error; 0.5-2 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
ml_flux_err_h
1 sigma flux error; 2.3-5 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.medium
double
ml_flux_err_u
1 sigma flux error; 5-8 keV
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.medium
double
ml_flux_lowerr_b1
1 sigma lower error of flux;0.2-0.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_lowerr_b2
1 sigma lower error of flux;0.5-1 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_lowerr_b3
1 sigma lower error of flux;1-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_lowerr_b4
1 sigma lower error of flux;2-4.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_lowerr_s
1 sigma lower error of flux;0.5-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_lowerr_h
1 sigma lower error of flux;2.3-5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_lowerr_u
1 sigma lower error of flux;5-8 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_uperr_b1
1 sigma upper error of flux;0.2-0.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_uperr_b2
1 sigma upper error of flux;0.5-1 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_uperr_b3
1 sigma upper error of flux;1-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_uperr_b4
1 sigma upper error of flux;2-4.5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_uperr_s
1 sigma upper error of flux;0.5-2 keV
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
ml_flux_uperr_h
1 sigma upper error of flux;2.3-5 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_flux_uperr_u
1 sigma upper error of flux;5-8 keV
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
ml_exp_b1
Vignetted exposure value; 0.2-0.5 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ml_exp_b2
Vignetted exposure value; 0.5-1 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ml_exp_b3
Vignetted exposure value; 1-2 keV
seconds
uctime.duration;obs.exposure;em.X-ray.soft
double
ml_exp_b4
Vignetted exposure value; 2-4.5 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ml_exp_s
Vignetted exposure value; 0.5-2 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ml_exp_h
Vignetted exposure value; 2.3-5 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ml_exp_u
Vignetted exposure value; 5-8 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ml_bkg_b1
Background at the source position; 0.2-0.5 keV
counts/arcmin^2
instr.background;em.X-ray.soft
double
ml_bkg_b2
Background at the source position; 0.5-1 keV
counts/arcmin^2
instr.background;em.X-ray.soft
double
ml_bkg_b3
Background at the source position; 1-2 keV
counts/arcmin^2
instr.background;em.X-ray.soft
double
ml_bkg_b4
Background at the source position; 2-4.5 keV
counts/arcmin^2
instr.background;em.X-ray.medium
double
ml_bkg_s
Background at the source position; 0.5-2 keV
counts/arcmin^2
instr.background;em.X-ray.soft
double
ml_bkg_h
Background at the source position; 2.3-5 keV
counts/arcmin^2
instr.background;em.X-ray.medium
double
ml_bkg_u
Background at the source position; 5-8 keV
counts/arcmin^2
instr.background;em.X-ray.medium
double
ape_cts_b1
Total counts extracted within the aperture; 0.2-0.5 keV
counts
phot.count;em.X-ray.soft
int
ape_cts_b2
Total counts extracted within the aperture; 0.5-1 keV
counts
phot.count;em.X-ray.soft
int
ape_cts_b3
Total counts extracted within the aperture; 1-2 keV
counts
phot.count;em.X-ray.soft
int
ape_cts_b4
Total counts extracted within the aperture; 2-4.5 keV
counts
phot.count;em.X-ray.medium
int
ape_cts_s
Total counts extracted within the aperture; 0.5-2 keV
counts
phot.count;em.X-ray.soft
int
ape_cts_h
Total counts extracted within the aperture; 2.3-5 keV
counts
phot.count;em.X-ray.medium
int
ape_cts_u
Total counts extracted within the aperture; 5-8 keV
counts
phot.count;em.X-ray.medium
int
ape_exp_b1
Vignetted exposure value; 0.2-0.5 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ape_exp_b2
Vignetted exposure value; 0.5-1 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ape_exp_b3
Vignetted exposure value; 1-2 keV
seconds
time.duration;obs.exposure;em.X-ray.soft
double
ape_exp_b4
Vignetted exposure value; 2-4.5 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ape_exp_s
Vignetted exposure value; 0.5-2 keV
seconds
uctime.duration;obs.exposured;em.X-ray.soft
double
ape_exp_h
Vignetted exposure value; 2.3-5 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ape_exp_u
Vignetted exposure value; 5-8 keV
seconds
time.duration;obs.exposure;em.X-ray.medium
double
ape_bkg_b1
Background counts in the aperture excluding nearby sources;
.2-.5keV
counts
instr.background;em.X-ray.soft
double
ape_bkg_b2
Background counts in the aperture excluding nearby sources;
0.5-1keV
counts
instr.background;em.X-ray.soft
double
ape_bkg_b3
Background counts in the aperture excluding nearby sources; 1-2
keV
counts
instr.backgrounde;em.X-ray.soft
double
ape_bkg_b4
Background counts in the aperture excluding nearby sources;
2-4.5keV
counts
instr.background;em.X-ray.medium
double
ape_bkg_s
Background counts in the aperture excluding nearby sources;
0.5-2keV
counts
instr.background;em.X-ray.soft
double
ape_bkg_h
Background counts in the aperture excluding nearby sources;
2.3-5keV
counts
instr.background;em.X-ray.medium
double
ape_bkg_u
Background counts in the aperture excluding nearby sources; 5-8
keV
counts
instr.background;em.X-ray.medium
double
ape_radius_b1
Aperture radius; 0.2-0.5 keV
pixels
phys.angSize;instr.pixel;em.X-ray.soft
double
ape_radius_b2
Aperture radius; 0.5-1 keV
pixels
phys.angSize;instr.pixel;em.X-ray.soft
double
ape_radius_b3
Aperture radius; 1-2 keV
pixels
phys.angSize;instr.pixel;em.X-ray.soft
double
ape_radius_b4
Aperture radius; 2-4.5 keV
pixels
phys.angSize;instr.pixel;em.X-ray.medium
double
ape_radius_s
Aperture radius; 0.5-2 keV
pixels
phys.angSize;instr.pixel;em.X-ray.soft
double
ape_radius_h
Aperture radius; 2.3-5 keV
pixels
phys.angSize;instr.pixel;em.X-ray.medium
double
ape_radius_u
Aperture radius; 5-8 keV
pixels
phys.angSize;instr.pixel;em.X-ray.medium
double
ape_pois_b1
Poisson probability of being background fluctuation; 0.2-0.5 keV
stat.probability;em.X-ray.soft
double
ape_pois_b2
Poisson probability of being background fluctuation; 0.5-1 keV
stat.probability;em.X-ray.soft
double
ape_pois_b3
Poisson probability of being background fluctuation; 1-2 keV
stat.probability;em.X-ray.soft
double
ape_pois_b4
Poisson probability of being background fluctuation; 2-4.5 keV
stat.probability;em.X-ray.medium
double
ape_pois_s
Poisson probability of being background fluctuation; 0.5-2 keV
stat.probability;em.X-ray.soft
double
ape_pois_h
Poisson probability of being background fluctuation; 2.3-5 keV
stat.probability;em.X-ray.medium
double
ape_pois_u
Poisson probability of being background fluctuation; 5-8 keV
stat.probability;em.X-ray.medium
double
catalogues.mv_erass1_hard_fdw
erass1_hard_oid
null
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
IAUNAME
String containing the official IAU name of the source
meta.id;meta.main
char
primary
DETUID
String unique detection ID
char
SKYTILE
Sky tile ID
int
ID_SRC
Source ID in each sky tile. Use SKYTILE+ID_SRC to identify the corresponding source products
int
UID
Integer unique detection ID. It equals CatID*10^11+SKYTILE*10^5+ID_SRC, where catID is 1 for the 1B detected Main and Supp catalogs and 2 for the 3B detected Hard catalog
long
UID_1B
1B catalog UID of the source with a strong association, or -UID if the association is weak
long
primary
ID_CLUSTER
Group ID of simultaneously fitted sources
int
RA
Right ascension (ICRS), corrected
deg
pos.eq.ra;meta.main
double
primary
DEC
Declination (ICRS), corrected
deg
pos.eq.dec;meta.main
double
primary
RA_RAW
Right ascension (ICRS), uncorrected
deg
double
DEC_RAW
Declination (ICRS), uncorrected
deg
double
RA_LOWERR
1-sigma lower error on RA
arcsec
double
RA_UPERR
1-sigma upper error on RA
arcsec
double
DEC_LOWERR
1-sigma lower error on DEC
arcsec
double
DEC_UPERR
1-sigma upper error on DEC
arcsec
double
POS_ERR
1-sigma positional uncertainty
double
RADEC_ERR
Combined positional error, raw output from PSF fitting
double
LII
deg
double
BII
deg
double
ELON
Ecliptic longitude
deg
double
ELAT
Ecliptic latitude
deg
double
MJD
Modified Julian Date of the observation of the source nearest to the optical axis of the telescope
double
MJD_MIN
Modified Julian Date of the first observation of the source
double
MJD_MAX
Modified Julian Date of the last observation of the source
double
EXT
Source Extent Parameter
arcsec
double
EXT_ERR
1-sigma error on EXT
arcsec
double
EXT_LOWERR
1-sigma lower error on EXT
arcsec
double
EXT_UPERR
1-sigma upper error on EXT
arcsec
double
EXT_LIKE
Extent likelihood
double
ML_CTS_0
Source net counts in 0.2-5.0 keV band
count
double
primary
ML_CTS_ERR_0
1-sigma combined counts error in 0.2-5.0 keV band
count
double
ML_RATE_0
Source count rate in 0.2-5.0 keV band
count s-1
double
ML_RATE_ERR_0
1-sigma combined count rate error in 0.2-5.0 keV band
count s-1
double
ML_FLUX_0
Source flux in 2.3-5.0 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_0
1-sigma combined error on flux in 0.2-5.0 keV band
erg s-1 cm-2
double
DET_LIKE_0
Detection likelihood in 0.2-5.0 keV band
double
ML_BKG_0
Background at the source position in the 0.2-5.0 keV band
arcmin-2
double
ML_CTS_1
Source net counts in 0.2-0.6 keV band
count
double
primary
ML_CTS_ERR_1
1-sigma combined counts error in 0.2-0.6 keV band
count
double
ML_CTS_LOWERR_1
1-sigma lower counts error in 0.2-0.6 keV band
count
double
ML_CTS_UPERR_1
1-sigma upper counts error in 0.2-0.6 keV band
count
double
ML_RATE_1
Source count rate in 0.2-0.6 keV band
count s-1
double
ML_RATE_ERR_1
1-sigma combined count rate error in 0.2-0.6 keV band
count s-1
double
ML_RATE_LOWERR_1
1-sigma lower count rate error in 0.2-0.6 keV band
count s-1
double
ML_RATE_UPERR_1
1-sigma upper count rate error in 0.2-0.6 keV band
count s-1
double
ML_FLUX_1
Source flux in 0.2-0.6 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_1
1-sigma combined error on flux in 0.2-0.6 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_1
1-sigma lower error on flux in 0.2-0.6 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_1
1-sigma upper error on flux in 0.2-0.6 keV band
erg s-1 cm-2
double
DET_LIKE_1
Detection likelihood in 0.2-0.6 keV band
double
ML_BKG_1
Background at the source position in the 0.2-0.6 keV band
arcmin-2
double
ML_EXP_1
Vignetted exposure time at the source position in 0.2-0.6 keV band
s
double
ML_EEF_1
Enclosed energy fraction in 0.2-0.6 keV band
double
APE_CTS_1
Total counts extracted within the aperture in 0.2-0.6 keV band
count
int
APE_BKG_1
Background counts extracted within the aperture in 0.2-0.6 keV band, excluding nearby sources using the source map
count
double
APE_EXP_1
Exposure map value in 0.2-0.6 keV band at the given position
s
double
APE_RADIUS_1
Extraction radius in pixels (4') in the 0.2-0.6 keV band
pix
double
APE_POIS_1
Poisson probability that the extracted counts (APE_CTS_1) are a background fluctuation
double
ML_CTS_2
Source net counts in 0.6-2.3 keV band
count
double
primary
ML_CTS_ERR_2
1-sigma combined counts error in 0.6-2.3 keV band
count
double
ML_CTS_LOWERR_2
1-sigma lower counts error in 0.6-2.3 keV band
count
double
ML_CTS_UPERR_2
1-sigma upper counts error in 0.6-2.3 keV band
count
double
ML_RATE_2
Source count rate in 0.6-2.3 keV band
count s-1
double
ML_RATE_ERR_2
1-sigma combined count rate error in 0.6-2.3 keV band
count s-1
double
ML_RATE_LOWERR_2
1-sigma lower count rate error in 0.6-2.3 keV band
count s-1
double
ML_RATE_UPERR_2
1-sigma upper count rate error in 0.6-2.3 keV band
count s-1
double
ML_FLUX_2
Source flux in 0.6-2.3 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_2
1-sigma combined error on flux in 0.6-2.3 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_2
1-sigma lower error on flux in 0.6-2.3 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_2
1-sigma upper error on flux in 0.6-2.3 keV band
erg s-1 cm-2
double
DET_LIKE_2
Detection likelihood in 0.6-2.3 keV band
double
ML_BKG_2
Background at the source position in the 0.6-2.3 keV band
arcmin-2
double
ML_EXP_2
Vignetted exposure time at the source position in 0.6-2.3 keV band
s
double
ML_EEF_2
Enclosed energy fraction in 0.6-2.3 keV band
double
APE_CTS_2
Total counts extracted within the aperture in 0.6-2.3 keV band
count
int
APE_BKG_2
Background counts extracted within the aperture in 0.6-2.3 keV band, excluding nearby sources using the source map
count
double
APE_EXP_2
Exposure map value in 0.6-2.3 keV band at the given position
s
double
APE_RADIUS_2
Extraction radius in pixels (4') in the 0.6-2.3 keV band
pix
double
APE_POIS_2
Poisson probability that the extracted counts (APE_CTS_2) are a background fluctuation
double
ML_CTS_3
Source net counts in 2.3-5.0 keV band
count
double
primary
ML_CTS_ERR_3
1-sigma combined counts error in 2.3-5.0 keV band
count
double
ML_CTS_LOWERR_3
1-sigma lower counts error in 2.3-5.0 keV band
count
double
ML_CTS_UPERR_3
1-sigma upper counts error in 2.3-5.0 keV band
count
double
ML_RATE_3
Source count rate in 2.3-5.0 keV band
count s-1
double
ML_RATE_ERR_3
1-sigma combined count rate error in 2.3-5.0 keV band
count s-1
double
ML_RATE_LOWERR_3
1-sigma lower count rate error in 2.3-5.0 keV band
count s-1
double
ML_RATE_UPERR_3
1-sigma upper count rate error in 2.3-5.0 keV band
count s-1
double
ML_FLUX_3
Source flux in 2.3-5.0 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_3
1-sigma combined error on flux in 2.3-5.0 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_3
1-sigma lower error on flux in 2.3-5.0 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_3
1-sigma upper error on flux in 2.3-5.0 keV band
erg s-1 cm-2
double
DET_LIKE_3
Detection likelihood in 2.3-5.0 keV band
double
ML_BKG_3
Background at the source position in the 2.3-5.0 keV band
arcmin-2
double
ML_EXP_3
Vignetted exposure time at the source position in 2.3-5.0 keV band
s
double
ML_EEF_3
Enclosed energy fraction in 2.3-5.0 keV band
double
APE_CTS_3
Total counts extracted within the aperture in 2.3-5.0 keV band
count
int
APE_BKG_3
Background counts extracted within the aperture in 2.3-5.0 keV band, excluding nearby sources using the source map
count
double
APE_EXP_3
Exposure map value in 2.3-5.0 keV band at the given position
s
double
APE_RADIUS_3
Extraction radius in pixels (4') in the 2.3-5.0 keV band
pix
double
APE_POIS_3
Poisson probability that the extracted counts (APE_CTS_3) are a background fluctuation
double
FLAG_SP_SNR
Source may lie within an overdense region near a supernova remnant
short
FLAG_SP_BPS
Source may lie within an overdense region near a bright point source
short
FLAG_SP_SCL
Source may lie within an overdense region near a stellar cluste
short
FLAG_SP_LGA
Source may lie within an overdense region near a local large galaxy
short
FLAG_SP_GC_CONS
Source may lie within an overdense region near a galaxy cluster
short
FLAG_NO_RADEC_ERR
Source contained no RADEC_ERR in the pre-processed version of the catalogue
short
FLAG_NO_EXT_ERR
Source contained no EXT_ERR in the pre-processed version of the catalogue
short
FLAG_NO_CTS_ERR
Source contained no CTS_ERR in the pre-processed version of the catalogue
short
FLAG_OPT
Source matched within 15' with a bright optical star, likely contaminated by optical loading
short
catalogues.mv_erass1_main_fdw
erass1_main_oid
null
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
IAUNAME
String containing the official IAU name of the source
meta.id;meta.main
char
primary
DETUID
String unique detection ID
char
SKYTILE
Sky tile ID
int
ID_SRC
Source ID in each sky tile. Use SKYTILE+ID_SRC to identify the corresponding source products
int
UID
Integer unique detection ID. It equals CatID*10^11+SKYTILE*10^5+ID_SRC, where catID is 1 for the 1B detected Main and Supp catalogs and 2 for the 3B detected Hard catalog
long
UID_Hard
Hard catalog UID of the source with a strong association, or -UID if the association is weak
long
primary
ID_CLUSTER
Group ID of simultaneously fitted sources
int
RA
Right ascension (ICRS), corrected
deg
pos.eq.ra;meta.main
double
primary
DEC
Declination (ICRS), corrected
deg
pos.eq.dec;meta.main
double
primary
RA_RAW
Right ascension (ICRS), uncorrected
deg
double
DEC_RAW
Declination (ICRS), uncorrected
deg
double
RA_LOWERR
1-sigma lower error on RA
arcsec
double
RA_UPERR
1-sigma upper error on RA
arcsec
double
DEC_LOWERR
1-sigma lower error on DEC
arcsec
double
DEC_UPERR
1-sigma upper error on DEC
arcsec
double
POS_ERR
1-sigma positional uncertainty
double
RADEC_ERR
Combined positional error, raw output from PSF fitting
double
LII
Galactic longitude
deg
double
BII
Galactic latitude
deg
double
ELON
Ecliptic longitude
deg
double
ELAT
Ecliptic latitude
deg
double
MJD
Modified Julian Date of the observation of the source nearest to the optical axis of the telescope
d
double
MJD_MIN
Modified Julian Date of the first observation of the source
d
double
MJD_MAX
Modified Julian Date of the last observation of the source
d
double
EXT
Source Extent Parameter
arcsec
double
EXT_ERR
1-sigma error on EXT
arcsec
double
EXT_LOWERR
1-sigma lower error on EXT
arcsec
double
EXT_UPERR
1-sigma upper error on EXT
arcsec
double
EXT_LIKE
Extent likelihood
double
DET_LIKE_0
Detection likelihood in 0.2-2.3 keV band
double
ML_CTS_1
Source net counts in 0.2-2.3 keV band
count
double
primary
ML_CTS_ERR_1
1-sigma combined counts error in 0.2-2.3 keV band
count
double
ML_CTS_LOWERR_1
1-sigma lower counts error in 0.2-2.3 keV band
count
double
ML_CTS_UPERR_1
1-sigma upper counts error in 0.2-2.3 keV band
count
double
ML_RATE_1
Source count rate in 0.2-2.3 keV band
count s-1
double
ML_RATE_ERR_1
1-sigma combined count rate error in 0.2-2.3 keV band
count s-1
double
ML_RATE_LOWERR_1
1-sigma lower count rate error in 0.2-2.3 keV band
count s-1
double
ML_RATE_UPERR_1
1-sigma upper count rate error in 0.2-2.3 keV band
count s-1
double
ML_FLUX_1
Source flux in 0.2-2.3 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_1
1-sigma combined error on flux in 0.2-2.3 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_1
1-sigma lower error on flux in 0.2-2.3 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_1
1-sigma upper error on flux in 0.2-2.3 keV band
erg s-1 cm-2
double
ML_BKG_1
Background at the source position in the 0.2-2.3 keV band
arcmin-2
double
ML_EXP_1
Vignetted exposure time at the source position in 0.2-2.3 keV band
s
double
ML_EEF_1
Enclosed energy fraction
double
APE_CTS_1
Total counts extracted within the aperture in 0.2-2.3 keV band
count
int
APE_BKG_1
Background counts extracted within the aperture in 0.2-2.3 keV band, excluding nearby sources using the source map
count
double
APE_EXP_1
Exposure map value in 0.2-2.3 keV band at the given position
s
double
APE_RADIUS_1
Extraction radius in pixels (4') in the 0.2-2.3 keV band
pix
double
APE_POIS_1
Poisson probability that the extracted counts (APE_CTS_1) are a background fluctuation
double
DET_LIKE_P1
Detection likelihood in 0.2-0.5 keV band
double
ML_CTS_P1
Source net counts in 0.2-0.5 keV band
count
double
primary
ML_CTS_ERR_P1
1-sigma combined counts error in 0.2-0.5 keV band
count
double
ML_CTS_LOWERR_P1
1-sigma lower counts error in 0.2-0.5 keV band
count
double
ML_CTS_UPERR_P1
1-sigma upper counts error in 0.2-0.5 keV band
double
ML_RATE_P1
Source count rate in 0.2-0.5 keV band
count s-1
double
ML_RATE_ERR_P1
1-sigma combined count rate error in 0.2-0.5 keV band
count s-1
double
ML_RATE_LOWERR_P1
1-sigma lower count rate error in 0.2-0.5 keV band
count s-1
double
ML_RATE_UPERR_P1
1-sigma upper count rate error in 0.2-0.5 keV band
double
ML_FLUX_P1
Source flux in 0.2-0.5 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P1
1-sigma combined flux error in 0.2-0.5 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P1
1-sigma lower flux error in 0.2-0.5 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_P1
1-sigma upper flux error in 0.2-0.5 keV band
erg s-1 cm-2
double
ML_BKG_P1
Background at the source position in 0.2-0.5 keV band
arcmin-2
double
ML_EXP_P1
Vignetted exposure time at the source position in 0.2-0.5 keV band
s
double
ML_EEF_P1
Enclosed energy fraction in 0.2-0.5 keV band
double
APE_CTS_P1
Total counts extracted within the aperture in 0.2-0.5 keV band
count
int
APE_BKG_P1
Background counts extracted within the aperture in 0.2-0.5 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P1
Exposure map value at the given position in the 0.2-0.5 keV band
s
double
APE_RADIUS_P1
Extraction radius in pixels (4') in the 0.2-0.5 keV band
pix
double
APE_POIS_P1
Poisson probability that the extracted counts (APE_CTS_P1) are a background fluctuation
double
DET_LIKE_P2
Detection likelihood in 0.5-1.0 keV band
double
ML_CTS_P2
Source net counts in 0.5-1.0 keV band
count
double
primary
ML_CTS_ERR_P2
1-sigma combined counts error in 0.5-1.0 keV band
count
double
ML_CTS_LOWERR_P2
1-sigma lower counts error in 0.5-1.0 keV band
count
double
ML_CTS_UPERR_P2
1-sigma upper counts error in 0.5-1.0 keV band
double
ML_RATE_P2
Source count rate in 0.5-1.0 keV band
count s-1
double
ML_RATE_ERR_P2
1-sigma combined count rate error in 0.5-1.0 keV band
count s-1
double
ML_RATE_LOWERR_P2
1-sigma lower count rate error in 0.5-1.0 keV band
count s-1
double
ML_RATE_UPERR_P2
1-sigma upper count rate error in 0.5-1.0 keV band
count s-1
double
ML_FLUX_P2
Source flux in 0.5-1.0 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P2
1-sigma combined flux error in 0.5-1.0 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P2
1-sigma lower flux error in 0.5-1.0 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_P2
1-sigma upper flux error in 0.5-1.0 keV band
erg s-1 cm-2
double
ML_BKG_P2
Background at the source position in 0.5-1.0 keV band
arcmin-2
double
ML_EXP_P2
Vignetted exposure time at the source position in 0.5-1.0 keV band
s
double
ML_EEF_P2
Enclosed energy fraction in 0.5-1.0 keV band
double
APE_CTS_P2
Total counts extracted within the aperture in 0.5-1.0 keV band
int
APE_BKG_P2
Background counts extracted within the aperture in 0.5-1.0 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P2
Exposure map value at the given position in the 0.5-1.0 keV band
s
double
APE_RADIUS_P2
Extraction radius in pixels (4') in the 0.5-1.0 keV band
pix
double
APE_POIS_P2
Poisson probability that the extracted counts (APE_CTS_P2) are a background fluctuation
double
DET_LIKE_P3
Detection likelihood in 1.0-2.0 keV band
double
ML_CTS_P3
Source net counts in 1.0-2.0 keV band
count
double
primary
ML_CTS_ERR_P3
1-sigma combined counts error in 1.0-2.0 keV band
count
double
ML_CTS_LOWERR_P3
1-sigma lower counts error in 1.0-2.0 keV band
count
double
ML_CTS_UPERR_P3
1-sigma upper counts error in 1.0-2.0 keV band
double
ML_RATE_P3
Source count rate in 1.0-2.0 keV band
count s-1
double
ML_RATE_ERR_P3
1-sigma combined count rate error in 1.0-2.0 keV band
count s-1
double
ML_RATE_LOWERR_P3
1-sigma lower count rate error in 1.0-2.0 keV band
count s-1
double
ML_RATE_UPERR_P3
1-sigma upper count rate error in 1.0-2.0 keV band
count s-1
double
ML_FLUX_P3
Source flux in 1.0-2.0 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P3
1-sigma combined flux error in 1.0-2.0 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P3
1-sigma lower flux error in 1.0-2.0 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_P3
1-sigma upper flux error in 1.0-2.0 keV band
erg s-1 cm-2
double
ML_BKG_P3
Background at the source position in 1.0-2.0 keV band
erg s-1 cm-2
double
ML_EXP_P3
Vignetted exposure time at the source position in 1.0-2.0 keV band
s
double
ML_EEF_P3
Enclosed energy fraction in 1.0-2.0 keV band
double
APE_CTS_P3
Total counts extracted within the aperture in 1.0-2.0 keV band
count
int
APE_BKG_P3
Background counts extracted within the aperture in 1.0-2.0 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P3
Exposure map value at the given position in the 1.0-2.0 keV band
s
double
APE_RADIUS_P3
Extraction radius in pixels (4') in the 1.0-2.0 keV band
pix
double
APE_POIS_P3
Poisson probability that the extracted counts (APE_CTS_P3) are a background fluctuation
double
DET_LIKE_P4
Detection likelihood in 2.0-5.0 keV band
double
ML_CTS_P4
Source net counts in 2.0-5.0 keV band
count
double
primary
ML_CTS_ERR_P4
1-sigma combined counts error in 2.0-5.0 keV band<
count
double
ML_CTS_LOWERR_P4
1-sigma lower counts error in 2.0-5.0 keV band
count
double
ML_CTS_UPERR_P4
1-sigma upper counts error in 2.0-5.0 keV band
double
ML_RATE_P4
Source count rate in 2.0-5.0 keV band
count s-1
double
ML_RATE_ERR_P4
1-sigma combined count rate error in 2.0-5.0 keV band
count s-1
double
ML_RATE_LOWERR_P4
1-sigma lower count rate error in 2.0-5.0 keV band
count s-1
double
ML_RATE_UPERR_P4
1-sigma upper count rate error in 2.0-5.0 keV band
count s-1
double
ML_FLUX_P4
Source flux in 2.0-5.0 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P4
1-sigma combined flux error in 2.0-5.0 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P4
1-sigma lower flux error in 2.0-5.0 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_P4
1-sigma upper flux error in 2.0-5.0 keV band
erg s-1 cm-2
double
ML_BKG_P4
Background at the source position in 2.0-5.0 keV band
arcmin-2
double
ML_EXP_P4
Vignetted exposure time at the source position in 2.0-5.0 keV band
s
double
ML_EEF_P4
Enclosed energy fraction in 2.0-5.0 keV band
double
APE_CTS_P4
Total counts extracted within the aperture in 2.0-5.0 keV band
count
int
APE_BKG_P4
Background counts extracted within the aperture in 2.0-5.0 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P4
Exposure map value at the given position in the 2.0-5.0 keV band
s
double
APE_RADIUS_P4
Extraction radius in pixels (4') in the 2.0-5.0 keV band
pix
double
APE_POIS_P4
Poisson probability that the extracted counts (APE_CTS_P4) are a background fluctuation
double
DET_LIKE_P5
Detection likelihood in 5.0-8.0 keV band
double
ML_CTS_P5
Source net counts in 5.0-8.0 keV band
count
double
primary
ML_CTS_ERR_P5
1-sigma combined counts error in 5.0-8.0 keV band
count
double
ML_CTS_LOWERR_P5
1-sigma lower counts error in 5.0-8.0 keV band
count
double
ML_CTS_UPERR_P5
1-sigma upper counts error in 5.0-8.0 keV band
double
ML_RATE_P5
Source count rate in 5.0-8.0 keV band
count s-1
double
ML_RATE_ERR_P5
1-sigma combined count rate error in 5.0-8.0 keV band
count s-1
double
ML_RATE_LOWERR_P5
1-sigma lower count rate error in 5.0-8.0 keV band
count s-1
double
ML_RATE_UPERR_P5
1-sigma upper count rate error in 5.0-8.0 keV band
count s-1
double
ML_FLUX_P5
Source flux in 5.0-8.0 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P5
1-sigma combined flux error in 5.0-8.0 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P5
1-sigma lower flux error in 5.0-8.0 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_P5
1-sigma upper flux error in 5.0-8.0 keV band
erg s-1 cm-2
double
ML_BKG_P5
Background at the source position in 5.0-8.0 keV band
arcmin-2
double
ML_EXP_P5
Vignetted exposure time at the source position in 5.0-8.0 keV band
s
double
ML_EEF_P5
Enclosed energy fraction in 5.0-8.0 keV band
double
APE_CTS_P5
Total counts extracted within the aperture in 5.0-8.0 keV band
count
int
APE_BKG_P5
Background counts extracted within the aperture in 5.0-8.0 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P5
Exposure map value at the given position in the 5.0-8.0 keV band
s
double
APE_RADIUS_P5
Extraction radius in pixels (4') in the 5.0-8.0 keV band
pix
double
APE_POIS_P5
Poisson probability that the extracted counts (APE_CTS_P5) are a background fluctuation
double
DET_LIKE_P6
Detection likelihood in 4.0-10.0 keV band
double
ML_CTS_P6
Source net counts in 4.0-10.0 keV band
count
double
primary
ML_CTS_ERR_P6
1-sigma combined counts error in 4.0-10.0 keV band
count
double
ML_CTS_LOWERR_P6
1-sigma lower counts error in 4.0-10.0 keV band
count
double
ML_CTS_UPERR_P6
1-sigma upper counts error in 4.0-10.0 keV band
double
ML_RATE_P6
Source count rate in 4.0-10.0 keV band
count s-1
double
ML_RATE_ERR_P6
1-sigma combined count rate error in 4.0-10.0 keV band
count s-1
double
ML_RATE_LOWERR_P6
1-sigma lower count rate error in 4.0-10.0 keV band
count s-1
double
ML_RATE_UPERR_P6
1-sigma upper count rate error in 4.0-10.0 keV band
count s-1
double
ML_FLUX_P6
Source flux in 4.0-10.0 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P6
1-sigma combined flux error in 4.0-10.0 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P6
1-sigma lower flux error in 4.0-10.0 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_P6
1-sigma upper flux error in 4.0-10.0 keV band
erg s-1 cm-2
double
ML_BKG_P6
Background at the source position in 4.0-10.0 keV band
arcmin-2
double
ML_EXP_P6
Vignetted exposure time at the source position in 4.0-10.0 keV band
s
double
ML_EEF_P6
Enclosed energy fraction in 4.0-10.0 keV band
double
APE_CTS_P6
Total counts extracted within the aperture in 4.0-10.0 keV band
count
int
APE_BKG_P6
Background counts extracted within the aperture in 4.0-10.0 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P6
Exposure map value at the given position in the 4.0-10.0 keV band
s
double
APE_RADIUS_P6
Extraction radius in pixels (4') in the 4.0-10.0 keV band
pix
double
APE_POIS_P6
Poisson probability that the extracted counts (APE_CTS_P6) are a background fluctuation
double
DET_LIKE_P7
Detection likelihood in 5.1-6.1 keV band
double
ML_CTS_P7
Source net counts in 5.1-6.1 keV band
count
double
primary
ML_CTS_ERR_P7
1-sigma combined counts error in 5.1-6.1 keV band
count
double
ML_CTS_LOWERR_P7
1-sigma lower counts error in 5.1-6.1 keV band
count
double
ML_CTS_UPERR_P7
1-sigma upper counts error in 5.1-6.1 keV band
double
ML_RATE_P7
Source count rate in 5.1-6.1 keV band
count s-1
double
ML_RATE_ERR_P7
1-sigma combined count rate error in 5.1-6.1 keV band
count s-1
double
ML_RATE_LOWERR_P7
1-sigma lower count rate error in 5.1-6.1 keV band
count s-1
double
ML_RATE_UPERR_P7
1-sigma upper count rate error in 5.1-6.1 keV band
count s-1
double
ML_FLUX_P7
Source flux in 5.1-6.1 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P7
1-sigma combined flux error in 5.1-6.1 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P7
1-sigma lower flux error in 5.1-6.1 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_P7
1-sigma upper flux error in 5.1-6.1 keV band
erg s-1 cm-2
double
ML_BKG_P7
Background at the source position in 5.1-6.1 keV band
arcmin-2
double
ML_EXP_P7
Vignetted exposure time at the source position in 5.1-6.1 keV band
s
double
ML_EEF_P7
Enclosed energy fraction in 5.1-6.1 keV band
double
APE_CTS_P7
Total counts extracted within the aperture in 5.1-6.1 keV band
count
int
APE_BKG_P7
Background counts extracted within the aperture in 5.1-6.1 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P7
Exposure map value at the given position in the 5.1-6.1 keV band
s
double
APE_RADIUS_P7
Extraction radius in pixels (4') in the 5.1-6.1 keV band
pix
double
APE_POIS_P7
Poisson probability that the extracted counts (APE_CTS_P7) are a background fluctuation
double
DET_LIKE_P8
Detection likelihood in 6.2-7.1 keV band
double
ML_CTS_P8
Source net counts in 6.2-7.1 keV band
count
double
primary
ML_CTS_ERR_P8
1-sigma combined counts error in 6.2-7.1 keV band
count
double
ML_CTS_LOWERR_P8
1-sigma lower counts error in 6.2-7.1 keV band
count
double
ML_CTS_UPERR_P8
1-sigma upper counts error in 6.2-7.1 keV band
double
ML_RATE_P8
Source count rate in 6.2-7.1 keV band
count s-1
double
ML_RATE_ERR_P8
1-sigma combined count rate error in 6.2-7.1 keV band
count s-1
double
ML_RATE_LOWERR_P8
1-sigma lower count rate error in 6.2-7.1 keV band
count s-1
double
ML_RATE_UPERR_P8
1-sigma upper count rate error in 6.2-7.1 keV band
count s-1
double
ML_FLUX_P8
Source flux in 6.2-7.1 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P8
1-sigma combined flux error in 6.2-7.1 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P8
1-sigma lower flux error in 6.2-7.1 keV band
erg s-1 cm-2
double
ML_FLUX_UPERR_P8
1-sigma upper flux error in 6.2-7.1 keV band
erg s-1 cm-2
double
ML_BKG_P8
Background at the source position in 6.2-7.1 keV band
arcmin-2
double
ML_EXP_P8
Vignetted exposure time at the source position in 6.2-7.1 keV band
s
double
ML_EEF_P8
Enclosed energy fraction in 6.2-7.1 keV band
double
APE_CTS_P8
Total counts extracted within the aperture in 6.2-7.1 keV band
count
int
APE_BKG_P8
Background counts extracted within the aperture in 6.2-7.1 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P8
Exposure map value at the given position in the 6.2-7.1 keV band
s
double
APE_RADIUS_P8
Extraction radius in pixels (4') in the 6.2-7.1 keV band
double
APE_POIS_P8
Poisson probability that the extracted counts (APE_CTS_P8) are a background fluctuation
pix
double
DET_LIKE_P9
Detection likelihood in 7.2-8.2 keV band
double
ML_CTS_P9
Source net counts in 7.2-8.2 keV band
count
double
primary
ML_CTS_ERR_P9
1-sigma combined counts error in 7.2-8.2 keV band
count
double
ML_CTS_LOWERR_P9
1-sigma lower counts error in 7.2-8.2 keV band
count
double
ML_CTS_UPERR_P9
1-sigma upper counts error in 7.2-8.2 keV band
double
ML_RATE_P9
Source count rate in 7.2-8.2 keV band
count s-1
double
ML_RATE_ERR_P9
1-sigma combined count rate error in 7.2-8.2 keV band
count s-1
double
ML_RATE_LOWERR_P9
1-sigma lower count rate error in 7.2-8.2 keV band
count s-1
double
ML_RATE_UPERR_P9
1-sigma upper count rate error in 7.2-8.2 keV band
count s-1
double
ML_FLUX_P9
Source flux in 7.2-8.2 keV band
erg s-1 cm-2
double
primary
ML_FLUX_ERR_P9
1-sigma combined flux error in 7.2-8.2 keV band
erg s-1 cm-2
double
ML_FLUX_LOWERR_P9
1-sigma lower flux error in 7.2-8.2 keV ban
erg s-1 cm-2
double
ML_FLUX_UPERR_P9
1-sigma upper flux error in 7.2-8.2 keV band
erg s-1 cm-2
double
ML_BKG_P9
Background at the source position in 7.2-8.2 keV band
arcmin-2
double
ML_EXP_P9
Vignetted exposure time at the source position in 7.2-8.2 keV band
s
double
ML_EEF_P9
Enclosed energy fraction in 7.2-8.2 keV band
double
APE_CTS_P9
Total counts extracted within the aperture in 7.2-8.2 keV band
count
int
APE_BKG_P9
Background counts extracted within the aperture in 7.2-8.2 keV band, excluding nearby sources using the source map
count
double
APE_EXP_P9
Exposure map value at the given position in the 7.2-8.2 keV band
s
double
APE_RADIUS_P9
Extraction radius in pixels (4') in the 7.2-8.2 keV band
pix
double
APE_POIS_P9
Poisson probability that the extracted counts (APE_CTS_P9) are a background fluctuation
double
APE_CTS_S
Total counts extracted within the aperture in 0.5-2.0 keV band
int
APE_BKG_S
Background counts extracted within the aperture in 0.5-2.0 keV band, excluding nearby sources using the source map
count
double
APE_EXP_S
Exposure map value at the given position in the 0.5-2.0 keV band
s
double
APE_POIS_S
Poisson probability that the extracted counts (APE_CTS_S) are a background fluctuation
double
FLAG_SP_SNR
Source may lie within an overdense region near a supernova remnant
short
FLAG_SP_BPS
Source may lie within an overdense region near a bright point source
short
FLAG_SP_SCL
Source may lie within an overdense region near a stellar cluster
short
FLAG_SP_LGA
Source may lie within an overdense region near a local large galaxy
short
FLAG_SP_GC_CONS
Source may lie within an overdense region near a galaxy cluster
short
FLAG_NO_RADEC_ERR
Source contained no RADEC_ERR in the pre-processed version of the catalogue
short
FLAG_NO_EXT_ERR
Source contained no EXT_ERR in the pre-processed version of the catalogue
short
FLAG_NO_CTS_ERR
Source contained no CTS_ERR in the pre-processed version of the catalogue
short
FLAG_OPT
Source matched within 15' with a bright optical star, likely contaminated by optical loading
short
catalogues.mv_etacha_c001_hard_fdw
etacha_c001_hard_oid
null
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
ero_name
eROSITA/SRG name
meta.id;meta.main
char
primary
id_src
Source ID
meta.id;src
int
id_main
Source ID in the main catalog
meta.id
int
ra
Right ascension
deg
pos.eq.ra;meta.main
double
primary
dec
Declination
deg
pos.eq.dec;meta.main
double
primary
radec_err
Combined positional error
arcsec
stat.error;pos
double
primary
ext
Source Extent
arcsec
phys.angSize;em.X-ray.medium
double
ext_err
Extent Error
arcsec
stat.error;phys.angSize;em.X-ray
double
ext_like
Extent Likelihood
stat.likelihood
double
ml_cts
Source counts from PSF-fitting
ct
phot.count
double
primary
ml_cts_err
1-sigma source counts error
ct
stat.error;phot.count;em.X-ray.medium
double
primary
ml_rate
Source rate from PSF-fitting
ct.s-1
arith.rate;phot.count
double
primary
ml_rate_err
1-sigma rate error
ct.s-1
stat.error;phot.count
double
primary
ml_flux
Source flux in the detection band
erg.s-1.cm-2
phot.flux;em.X-ray
double
primary
ml_flux_err
1-sigma source flux error
erg.s-1.cm-2
phot.flux;em.X-ray.medium
double
primary
det_like
Detection likelihood
stat.likelihood
double
primary
ml_bkg
Background at the source position
ct.arcmin-2
instr.background
double
primary
catalogues.mv_etacha_c001_main_fdw
etacha_c001_main_oid
null
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
ero_name
eROSITA/SRG name
meta.id;meta.main
char
primary
id_src
Source ID
meta.id;src
int
ra
Right ascension
deg
pos.eq.ra;meta.main
double
primary
dec
Declination
deg
pos.eq.dec;meta.main
double
primary
radec_err
Combined positional error
arcsec
stat.error;pos
double
primary
ext
Source Extent
arcsec
phys.angSize;em.X-ray.soft
double
ext_err
Extent Error
arcsec
stat.error;phys.angSize;em.X-ray.soft
double
ext_like
Extent Likelihood
stat.likelihood
double
ml_cts
Source counts from PSF-fitting
cts
phot.count;em.X-ray.soft
double
primary
ml_cts_err
1-sigma source counts error
cts
stat.error;phot.count;em.X-ray.soft
double
primary
ml_rate
Source rate from PSF-fitting
ct.s-1
arith.rate;phot.count
double
primary
ml_rate_err
1-sigma rate error
ct.s-1
stat.error;phot.count
double
primary
ml_flux
Source flux in the detection band
erg.s-1.cm-2
phot.flux;em.X-ray.soft
double
primary
ml_flux_err
1-sigma source flux error
erg.s-1.cm-2
stat.error;phot.flux;em.X-ray.soft
double
primary
det_like
Detection likelihood
stat.likelihood
double
primary
ml_bkg
Background at the source position
ct.arcmin-2
instr.background
double
primary
catalogues.mv_euclid_mer_catalogue
npix
int
object_id
Euclid unique source identifier
NA
long
primary
right_ascension
Source barycenter RA coordinate (SExtractor ALPHA_J2000) decimal degrees
deg
pos.eq.ra;meta.main
double
primary
declination
Source barycenter DEC coordinate (SExtractor DELTA_J2000) decimal degrees
deg
pos.eq.dec;meta.main
double
primary
flux_detection_total
VIS or NIR stack band source total flux error (Kron aperture)
uJy
double
primary
det_quality_flag
Detection step flags that could indicate the possible corruption of the MAG_STARGAL_SEP values
NA
short
primary
vis_det
Flag to indicate if the source is detected in the VIS mosaic (1) or is only detected in the NIR mosaic (0)
NA
short
primary
flux_vis_sersic
VIS band source flux from the Sersic fit
uJy
double
primary
flux_y_sersic
NIR Y band source flux from the Sersic fit
uJy
double
primary
flux_j_sersic
NIR J band source flux from the Sersic fit
uJy
double
primary
flux_h_sersic
NIR H band source flux from the Sersic fit
uJy
double
primary
segmentation_area
Isophotal area of the source above the analysis threshold (SExtractor ISOAREA_IMAGE)
pix
int
primary
segmentation_map_id
Source ID in the associated segmentation map
NA
long
primary
kron_radius
Major semi-axis (in pixels) of the elliptical aperture used for total (Kron) aperture photometry on the detection image
pix
double
primary
catalogues.mv_fermi_3fhl_fdw
fermi_3fhl_oid
meta.oid
int
stc_s
STCS representation of the area covered byt the 95% error ellipse
obscore:Char.SpatialAxis.Coverage.Support.Area
char
npix
Healpix pixel of the center of the observation for nside 256
long
recno
Record number assigned by the VizieR team. Should Not be used for identification.
meta.record
int
"3fhl"
3FHL name (JHHMM.m+DDMMe) (Source_Name)
meta.id;meta.main
char
ra
Right ascension; J2000 (RAJ2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination; J2000 (DEJ2000)
deg
pos.eq.dec;meta.main
double
primary
glon
Galactic longitude (GLON)
deg
pos.galactic.lon
double
glat
Galactic latitude (GLAT)
deg
pos.galactic.lat
double
c95amaj
[0.008/0.2]? Error radius at 95% confidence (Conf_95_SemiMajor)
deg
stat.error
double
c95bmin
[0.008/0.2]? Conf_95_SemiMajor in 3FHL (Conf_95_SemiMinor)
deg
stat.error
double
c95pa
[-1e+38]? error circle; NULL in 3FHL (Conf_95_PosAng)
deg
stat.error
double
roi
[1/728] ROI number (ROI_num)
meta.id
short
sig
[4/169] Source significance in {sigma} units over the 10GeV to 2TeV band (Signif_Avg)
stat.fit.goodness;arith.ratio
double
primary
epvt
[11/195] Energy at which error on differential flux is minimal (Pivot_Energy)
GeV
phys.energy
double
primary
s
Differential flux at Pivot_Energy (Flux_Density)
ph/cm2/GeV/s
phot.flux;arith.ratio
double
primary
e_s
1{sigma} error on S (Unc_Flux_Density)
ph/cm2/GeV/s
stat.error
double
flux
Integral photon flux from 10GeV to 1TeV obtained by spectral fitting (Flux)
ph/cm2/s
phot.flux.density;em.gamma.hard
double
primary
e_flux
1{sigma} error on Flux (Unc_Flux)
ph/cm2/s
stat.error;phot.flux
double
eflx
Energy flux from 10GeV to 1TeV obtained by spectral fitting; in erg/cm^2^/s (Energy_Flux)
10-3W/m2
phot.flux.density;em.gamma.hard
double
primary
e_eflx
1{sigma} error on EFlx (Unc_Energy_Flux)
10-3W/m2
stat.error
double
sigcve
[0/6] Significance (in {sigma} units) of the fit improvement between power-law and LogParabola (Signif_Curve) (1)
stat.fit.goodness
double
spt
Spectral type (PowerLaw or LogParabola); see section 2.4 (SpectrumType)
src.spType
char
sind
[0.9/9.1] Best-fit photon number index at Pivot_Energy when fitting with LogParabola (Spectral_Index)
spect.index
double
e_sind
[0.04/4.1] 1{sigma} error on SInd (Unc_Spectral_Index)
spect.index
double
beta
[-0.8/1] Curvature parameter {beta} when fitting with LogParabola (beta)
stat.fit.param
double
e_beta
[0.001/9.3] 1{sigma} error on beta (Unc_beta)
stat.error
double
plind
[1/9.1] Best-fit photon number index when fitting with power law (PowerLaw_Index)
spect.index
double
e_plind
[0.02/4] 1{sigma} error on PLInd (Unc_PowerLaw_Index)
spect.index
double
f1
Integral photon flux in 10-20GeV spectral band (Flux_Band1)
ph/cm2/s
phot.flux
double
primary
e_upper_f1
? 1{sigma} upper error on F1 (Low_Unc_Flux_Band2) (2)
ph/cm2/s
stat.error;stat.max
double
e_lower_f1
? 1{sigma} lower error on F1 (Low_Unc_Flux_Band1) (2)
ph/cm2/s
stat.error
double
f2
Integral photon flux in 20-50GeV spectral band (Flux_Band2)
ph/cm2/s
phot.flux
double
primary
e_upper_f2
? 1{sigma} upper error on F2 (Low_Unc_Flux_Band4) (2)
ph/cm2/s
stat.error;stat.max
double
e_lower_f2
? 1{sigma} lower error on F2 (Low_Unc_Flux_Band3) (2)
ph/cm2/s
stat.error
double
f3
[0/] Integral photon flux in 50-150GeV spectral band (Flux_Band3)
ph/cm2/s
phot.flux
double
primary
e_upper_f3
? 1{sigma} upper error on F3 (Up_Unc_Flux_Band1) (2)
ph/cm2/s
stat.error;stat.max
double
e_lower_f3
? 1{sigma} lower error on F3 (Low_Unc_Flux_Band5) (2)
ph/cm2/s
stat.error
double
f4
[0/] Integral photon flux in 150-500GeV spectral band (Flux_Band4)
ph/cm2/s
phot.flux
double
primary
e_upper_f4
? 1{sigma} upper error on F4 (Up_Unc_Flux_Band3) (2)
ph/cm2/s
stat.error;stat.max
double
e_lower_f4
? 1{sigma} lower error on F4 (Up_Unc_Flux_Band2) (2)
ph/cm2/s
stat.error
double
f5
[0/] Integral photon flux in 500-2000GeV spectral band (Flux_Band5)
ph/cm2/s
phot.flux
double
primary
e_upper_f5
? 1{sigma} upper error on F5 (Up_Unc_Flux_Band5) (2)
ph/cm2/s
stat.error;stat.max
double
e_lower_f5
? 1{sigma} lower error on F5 (Up_Unc_Flux_Band4) (2)
ph/cm2/s
stat.error
double
nufnu1
Spectral energy distribution in 10-20GeV, in erg/cm^2^/s (nuFnu1)
10-3W/m2
phot.flux
double
nufnu2
Spectral energy distribution in 20-50GeV, in erg/cm^2^/s (nuFnu2)
10-3W/m2
phot.flux
double
primary
nufnu3
[0/] Spectral energy distribution in 50-150GeV, in erg/cm^2^/s (nuFnu3)
10-3W/m2
phot.flux
double
primary
nufnu4
[0/] Spectral energy distribution in 150-500GeV, in erg/cm^2^/s (nuFnu4)
10-3W/m2
phot.flux
double
primary
nufnu5
[0/] Spectral energy distribution in 500-2000GeV, in erg/cm^2^/s (nuFnu5)
10-3W/m2
phot.flux
double
primary
ts1
[0/134] Square root of the Test Statistic in 10-20GeV (Sqrt_TS_Band1)
stat.fit.goodness
double
ts2
[0/89] Square root of the Test Statistic in 20-50GeV (Sqrt_TS_Band2)
stat.fit.goodness
double
ts3
[0/60] Square root of the Test Statistic in 50-150GeV (Sqrt_TS_Band3)
stat.fit.goodness
double
ts4
[0/34] Square root of the Test Statistic in 150-500GeV (Sqrt_TS_Band4)
stat.fit.goodness
double
ts5
[0/16] Square root of the Test Statistic in 500-2000GeV (Sqrt_TS_Band5)
stat.fit.goodness
double
npred
[4/3734] Predicted number of events in the model (Npred)
meta.number
double
hepe
[11.9/1997] Highest energy among events probably coming from the source (HEP_Energy)
GeV
phys.energy;stat.max
double
hepp
Probability of that event to come from the source (HEP_Prob)
stat.fit.goodness
double
var
[1/15]? Number of Bayesian blocks from variability analysis (1=not variable) (Variability_BayesBlocks)
meta.number
short
primary
exname
Cross-reference to the ExtendedSources extension (Extended_Source_Name)
meta.id.assoc
char
primary
assoc
Correspondence to previous {gamma}-ray source catalog (ASSOC_GAM) (3)
meta.id.assoc
char
primary
f_tname
TeVCat flag (TEVCAT_FLAG) (4)
meta.code
char
tname
Name of likely corresponding TeV source from TeVCat, if any (ASSOC_TEV)
meta.id.assoc
char
cl
Class designation for associated source see Table 2 (CLASS) (5)
meta.code.class
char
primary
assoc1
Name of identified or likely associated source (ASSOC1)
meta.id.assoc
char
primary
assoc2
Alternate name or indicates whether the source is inside an extended source
meta.id.assoc
char
pbay
? Probability of association according to the Bayesian method (ASSOC_PROB_BAY)
stat.fit.goodness
double
plr
? Probability of association according to the Likelihood-Ratio method (ASSOC_PROB_LR)
stat.fit.goodness
double
z
[0.003/2.6]? Redshift of counterpart, if known (Redshift)
src.redshift
double
nupk
? Frequency of the synchrotron peak of counterpart, if known (NuPeak_obs)
Hz
em.freq
double
catalogues.mv_fermi_4fgl_dr2_fdw
source_name
Source name 4FGL JHHMM.m+DDMMa
meta.id;meta.main
char
datarelease
double
ra
Right Ascension J2000
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000
deg
pos.eq.dec;meta.main
double
primary
glon
Galactic Longitude
deg
pos.galactic.lon
double
glat
Galactic Latitude
deg
pos.galactic.lat
double
conf_68_semimajor
Long radius of error ellipse at 68% confidence
deg
pos;stat.error
double
conf_68_semiminor
Short radius of error ellipse at 68% confidence
deg
pos;stat.error
double
conf_68_posang
Position angle of the 68% ellipse
deg
phys.angSize;stat.error
double
conf_95_semimajor
Long radius of error ellipse at 95% confidence
deg
pos;stat.error
double
conf_95_semiminor
Short radius of error ellipse at 95% confidence
deg
pos;stat.error
double
conf_95_posang
Position angle (eastward) of the long axis from celestial North
deg
phys.angSize;stat.error
double
roi_num
RoI number (cross-reference to ROIs extension)
double
extended_source_name
Cross-reference to the ExtendedSources extension
char
signif_avg
Source significance in σ units over the 100 MeV to 1 TeV band
stat.snr
double
primary
pivot_energy
Energy at which error on differential flux is minimal
MeV
em.energy
double
flux1000
Integral photon flux from 1 to 100GeV
ph cm-2 s-1
phot.count;em.gamma
double
primary
unc_flux1000
1σ error on integral photon flux from 1 to 100 GeV
ph cm-2 s-1
phot.count;em.gamma;stat.error
double
primary
energy_flux100
Energy flux from 100 MeV to 100 GeV obtained by spectral fitting
erg cm-2 s-1
phot.flux;em.gamma
double
unc_energy_flux100
1σ error on energy flux from 100 MeV to 100 GeV
erg cm-2 s-1
phot.flux;em.gamma;stat.error
double
spectrumtype
Spectral type in the global model (PowerLaw, LogParabola, PLSuperExpCutoff)
char
pl_flux_density
Differential flux at Pivot_Energy in PowerLaw fit
ph cm-2 MeV-1 s-1
phot.flux.density
double
unc_pl_flux_density
1σ error on PL_Flux_Density
ph cm-2 MeV-1 s-1
phot.flux.density;stat.error
double
pl_index
Photon index when fitting with PowerLaw
spect.index
double
unc_pl_index
1σ error on PL_Index
spect.index;stat.error
double
lp_flux_density
Differential flux at Pivot_Energy in LogParabola fit
ph cm-2 MeV-1 s-1
phot.flux.density
double
unc_lp_flux_density
1σ error on LP_Flux_Density
ph cm-2 MeV-1 s-1
phot.flux.density;stat.error
double
lp_index
Photon index at Pivot_Energy when fitting with LogParabola
spect.index
double
unc_lp_index
1σ error on LP_Index
spect.index;stat.error
double
lp_beta
Curvature parameter when fitting with LogParabola
double
unc_lp_beta
1σ error on LP_beta
double
lp_sigcurv
Significance (in σ units) of the fit improvement between PowerLaw and LogParabola. A value greater than 4 indicates significant curvature
stat.snr
double
plec_flux_density
Differential flux at Pivot_Energy in PLSuperExpCutoff fit
ph cm-2 MeV-1 s-1
phot.flux.density
double
unc_plec_flux_density
1σ error on PLEC_Flux_Density
ph cm-2 MeV-1 s-1
phot.flux.density;stat.error
double
plec_index
Low-energy photon index (Γ of Equation (4)) when fitting with PLSuperExpCutoff
spect.index
double
unc_plec_index
1σ error on PLEC_Index
spect.index;stat.error
double
plec_expfactor
Exponential factor when fitting with PLSuperExpCutoff
double
unc_plec_expfactor
1σ error on PLEC_Expfactor
double
plec_exp_index
Exponential index when fitting with PLSuperExpCutoff
double
unc_plec_exp_index
1σ error on PLEC_Exp_Index
double
plec_sigcurv
Same as LP_SigCurv for PLSuperExpCutoff model
stat.snr
double
npred
Predicted number of events in the model
double
flux_band
Integral photon flux in each spectral band
ph cm-2 s-1
phot.count;em.gamma
char
unc_flux_band
1σ lower and upper error on Flux_Band
ph cm-2 s-1
phot.count;em.gamma;stat.error
char
nufnu_band
Spectral energy distribution over each spectral band
erg cm-2 s-1
phot.flux.density;em.gamma
char
sqrt_ts_band
Square root of the Test Statistic in each spectral band
stat.snr
char
variability_index
Sum of 2×log(Likelihood) difference between the flux fitted in each time
interval and the average flux over the full catalog interval; a value greater
than 18.48 over 12 intervals indicates <1% chance of being a steady source
src.var.index;stat.chi2
double
frac_variability
Fractional variability computed from the fluxes in each year
src.var.amplitude
double
primary
unc_frac_variability
1σ error on fractional variability
src.var.amplitude;stat.error
double
signif_peak
Source significance in peak interval in σ units
stat.snr
double
flux_peak
Peak integral photon flux from 100 MeV to 100 GeV
ph cm-2 s-1
phot.count;em.gamma
double
unc_flux_peak
1σ error on peak integral photon flux
ph cm-2 s-1
phot.count;em.gamma;stat.error
double
time_peak
Time of center of interval in which peak flux was measured
s
time.epoch
double
peak_interval
Length of interval in which peak flux was measured
s
time.interval
double
flux_history
Integral photon flux from 100 MeV to 100 GeV in each year (best fit from likelihood analysis with spectral shape fixed to that obtained over full interval)
ph cm-2 s-1
phot.count;em.gamma
char
unc_flux_history
1σ lower and upper error on integral photon flux in each year
ph cm-2 s-1
phot.count;em.gamma;stat.error
char
sqrt_ts_history
Square root of the Test Statistic in each year
stat.snr
char
assoc_fgl
Most recent correspondence to previous FGL source catalogs, if any
meta.id.assoc
char
assoc_fhl
Most recent correspondence to previous FHL source catalogs, if any
meta.id.assoc
char
assoc_gam1
Name of likely corresponding 2AGL source, if any
meta.id.assoc
char
assoc_gam2
Name of likely corresponding 3EG source, if any
meta.id.assoc
char
assoc_gam3
Name of likely corresponding EGR source, if any
meta.id.assoc
char
tevcat_flag
P if positional association with non-extended source in TeVCat
E if associated with an extended source in TeVCat, N if no TeV association
meta.code
char
primary
assoc_tev
Name of likely corresponding TeV source from TeVCat, if any
meta.id.assoc
char
primary
class1
Class designation for associated source
src.class
char
primary
class2
Class designation for low-confidence association
src.class
char
assoc1
Name of identified or likely associated source
meta.id.assoc
char
primary
assoc2
Name of low-confidence association or of enclosing extended source
meta.id.assoc
char
assoc_prob_bay
Probability of association according to the Bayesian method
stat.probability
double
assoc_prob_lr
Probability of association according to the Likelihood Ratio method
stat.probability
double
ra_counterpart
R.A. of the counterpart ASSOC1
deg
pos.eq.ra
double
dec_counterpart
decl. of the counterpart ASSOC1
deg
pos.eq.dec
double
unc_counterpart
95% precision of the counterpart localization
deg
pos;stat.error
double
flags
Source flags (binary coding as in Table 5)
meta.code.qual
double
fermi_4fgl_dr2_oid
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
stc_s
STCS representation of the area covered byt the 68% error ellipse
obscore:Char.SpatialAxis.Coverage.Support.Area
char
catalogues.mv_fermi_4lac_fdw
fermi_4lac_oid
meta.oid
int
"group"
char
primary
"mod"
char
npix
Healpix pixel of the center of the observation for nside 256
long
recno
Record number assigned by the VizieR team. Should Not be used for identification.
meta.record
int
"4fgl"
4FGL name (JHHMM.m+DDMMa) (Source_Name)
meta.id;meta.main
char
ra
Right ascension (J2000) (RAJ2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination (J2000) (DEJ2000)
deg
pos.eq.dec;meta.main
double
primary
glon
Galactic longitude
deg
pos.galactic.lon
double
glat
Galactic latitude
deg
pos.galactic.lat
double
sig
[4/444] Source significance in {sigma} units over the 50MeV-1TeV band (Signif_Avg)
stat.fit.goodness;arith.ratio
double
f1000i
[8.8e-12/9.9e-8] Integral photon flux from 1 to 100GeV (Flux1000)
ph/cm2/s
phot.flux.density;em.gamma.hard
double
primary
e_f1000i
[4.9e-12/6e-10] F1000i 1{sigma} error (Unc_Flux1000)
ph/cm2/s
stat.error
double
ef100
[6.4e-13/1.2e-9] Energy flux from 100MeV to 100GeV obtained by spectral fitting in erg/cm^2^/s units (Energy_Flux100)
mW/m2
phot.flux.density;em.gamma.hard
double
primary
e_ef100
[1.7e-13/6.5e-12] EF100 1{sigma} error (Unc_Energy_Flux100)
mW/m2
stat.error
double
plgam
[1.39/3.5] Photon index when fitting with PowerLaw (PL_Index)
spect.index
double
e_plgam
[0.003/0.33] PLGam 1{sigma} error (Unc_PL_Index)
stat.error
double
epiv
[137.8/25099.3] Pivot Energy (Pivot_Energy)
MeV
phys.energy
double
lpalpha
[-0.34/3.6] Photon index at Pivot_Energy ({alpha}) when fitting with LogParabola (LP_Index)
spect.index
double
e_lpalpha
[0.004/3] LPalpha 1{sigma} error (Unc_LP_Index)
stat.error
double
lpbeta
[-0.17/1] Curvature parameter ({beta}) when fitting with LogParabola (LP_beta)
stat.fit.param
double
e_lpbeta
[0.001/1.5]? LPbeta 1{sigma} error (Unc_LP_beta)
stat.error
double
flags
[0/2096] Analysis flags (0=no warning)
meta.code.error
short
class
Class designation for associated source
src.class
char
primary
assoc1
Name of identified or likely associated source
meta.id.assoc
char
probby
[0/1]? Probability of association according to the Bayesian method (ASSOC_PROB_BAY)
stat.fit.goodness
double
primary
problr
[0/1] Probability of association according to the Likelihood Ratio method (ASSOC_PROB_LR)
stat.fit.goodness
double
primary
ccat
Counterpart catalog driving the association (Counterpart_Catalog) (1)
meta.id;meta.dataset
char
primary
racdeg
Right ascension of the counterpart Assoc1 (J2000) (RA_Counterpart)
deg
pos.eq.ra
double
decdeg
Declination of the counterpart Assoc1 (J2000) (DEC_Counterpart)
deg
pos.eq.dec
double
errcpos
[3.8e-8/2.5] 95% precision of the counterpart localization (Unc_Counterpart)
deg
meta.code.qual;instr.precision
double
rfc
Name of the VLBI counterpart (JHHMM+DDMM) (VLBI_Counterpart)
meta.id.cross
char
primary
gaia
? Name of the Gaia DR2 counterpart established via the VLBI position (Gaia_Counterpart)
meta.id.cross
char
primary
gmag
[12.8/21.5]? Gaia G-band magnitude (Gaia_G_Magnitude)
mag
phot.mag;em.opt
double
z
[1.7e-5/4.4]? Redshift (Redshift)
src.redshift
double
primary
sedcl
SED-based class (HSP, ISP or LSP) (SED_class)
src.spType
char
primary
nu
[0/1.2e+19] Synchrotron-peak frequency in observer frame (nu_syn)
Hz
em.freq;obs.field
double
nufnu
[0/7.9e-10] Spectral energy distribution at synchrotron-peak frequency in erg/cm^2^/s units (nuFnu_syn)
mW/m2
phot.flux.density;em.gamma.hard
double
primary
var
[0.3/50906] Variability index (Variability_Index)
src.var.index
double
fvar
[0/2.6] Fractional variability (Frac_Variability)
src.var.index
double
primary
e_fvar
[0.02/10] FVar 1{sigma} error (Unc_Frac_Variability)
stat.error
double
emax
[4.1/913]? Energy of the highest-energy ULTRACLEANVETO photon with association probability P>0.95 (Highest_energy)
GeV
double
primary
vhe
Display data for this Very-High-Energy AGN (link to Table 7)
meta.ref.url
short
pec
Display data for this non-blazar object (link to Table 6)
meta.ref.url
short
catalogues.mv_glade_plus_fdw
glade_no
GLADE+ catalog number
meta.id;meta.main
int
indexed
primary
pgc_no
Principal Galaxies Catalogue number
meta.id
int
gwgc_name
Name in the GWGC catalog
meta.id
char
hyperleda_name
Name in the HyperLEDA catalog
meta.id
char
"2mass_name"
Name in the 2MASS XSC catalog
meta.id
char
wisexscos_name
Name in the WISExSuperCOSMOS catalog (wiseX)
meta.id
char
"sdss-dr16q_name"
Name in the SDSS-DR16Q catalog
meta.id
char
object_type_flag
Q: the source is from the SDSS-DR16Q catalog; G: the source is from another catalog and has not been identified as a quasar
char
ra
Right ascension in degrees
degree
pos.eq.ra;meta.main
Char.SpatialAxis.Coverage.Location.Value.C1
double
primary
dec
Declination in degrees
degree
pos.eq.dec;meta.main
Char.SpatialAxis.Coverage.Location.Value.C2
double
primary
b
Apparent B magnitude
mag
phot.mag;em.opt.B
double
primary
b_err
Absolute error of apparent B magnitude
mag
phot.mag;em.opt.B
double
b_flag
0: the B magnitude is measured; 1: the B magnitude is calculated from the B_J magnitude
short
b_abs
Absolute B magnitude
mag
phys.magAbs:em.opt.B
double
j
Apparent J magnitude
mag
phot.mag;em.IR.J
double
primary
j_err
Absolute error of apparent J magnitude
mag
phot.mag;em.IR.J
double
h
Apparent H magnitude
mag
phot.mag;em.IR.H
double
primary
h_err
Absolute error of apparent H magnitude
mag
phot.mag;em.IR.H
double
k
Apparent K_s magnitude
mag
phot.mag;em.IR.K
double
primary
k_err
Absolute error of apparent K_s magnitude
mag
phot.mag;em.IR.K
double
w1
Apparent W1 magnitude
mag
phot.mag;em.IR.3-4um
double
primary
w1_err
Absolute error of apparent W1 magnitude
mag
phot.mag;em.IR.3-4um
double
w2
Apparent W2 magnitude
mag
phot.mag;em.IR.4-8um
double
primary
w2_err
Absolute error of apparent W2 magnitude
mag
phot.mag;em.IR.4-8um
double
w1_flag
0: the W1 magnitude is measured; 1: the W1 magnitude is calculated from the K_s magnitude
short
b_j
Apparent B_j magnitude
mag
phot.mag;em.opt.B
double
primary
b_j_err
Absolute error of apparent B_j magnitude
mag
phot.mag;em.opt.B
double
z_helio
Redshift in the heliocentric frame
src.redshift;pos.heliocentric
double
z_cmb
Redshift converted to the Cosmic Microwave Background (CMB) frame
src.redshift;pos.cmb
double
z_flag
0: the CMB frame redshift and luminosity distance values given in columns 29 and 33 are not corrected for the peculiar velocity; 1: they are corrected values
short
v_err
Error of redshift from the peculiar velocity estimation
double
z_err
Measurement error of heliocentric redshift
stat.error;src.redshift
double
d_l
Luminosity distance in Mpc units
Mpc
pos.distance
double
primary
d_l_err
Error of luminosity distance in Mpc units
Mpc
stat.error;pos.distance
double
dist_flag
0: the galaxy has no measured redshift or distance value; 1: it has a measured photometric redshift from which we have calculated its luminosity distance; 2: it has a measured luminosity distance value from which we have calculated its redshift; 3: it has a measured spectroscopic redshift from which we have calculated its luminosity distance
short
m_msun
Stellar mass in 10^10 M_Sun units
solMass
phys.mass
double
m_msun_err
Absolute error of stellar mass in 10^10 M_Sun units
solMass
phys.mass
double
m_msun_flag
0: if the stellar mass was calculated assuming no active star formation; 1: if the stellar mass was calculated assuming active star formation
short
merger_rate
Base-10 logarithm of estimated BNS merger rate in the galaxy in Gyr^-1 units
Gyr-1
double
merger_rate_error
Absolute error of estimated BNS merger rate in the galaxy
Gyr-1
double
catalogues.mv_hcv_catalogue
min_hcv_mag
Min value for HCV Magnitude
mag
double
npix
int
primary
matchid
Match Identifier of the Source (MatchId in HSCv3).
int
primary
groupid
Unique identifier for the image group of overlapping images.
int
primary
subgroup
Subgroup identifier. Very large groups have been split into subgroups. A value of "-5" denotes that the GroupID was processed as one subgroup.
int
primary
ra
Right ascension coordinate (J2000) of matched position (degrees).
deg
pos.eq.ra;meta.main
double
primary
dec
Declination coordinate (J2000) of matched position (degrees).
deg
pos.eq.dec;meta.main
double
primary
pipeline_class
A pipeline classification "1" corresponds to a single-filter variable candidate (SFVC), while "2" corresponds to a multi-filter variable candidate (MFVC).
int
primary
expert_class
The expert classification flag: "0" indicates a variable candidate "not classified by the expert", "1" indicates a "high confidence variable", "2" indicates a "probable variable", "4" indicates a "possible artifact".
int
primary
num_filters
Number of filters in which the source has been observed.
int
primary
filter
Instrument and filter name.
char
primary
num_in_lc
Number of points (epochs) in the light curve.
char
primary
var_quality_flag
Five letter quality flag for the source variability. Quantifies the deviation of each parameter (CI, D, MagerrAper2, MagAper2-MagAuto, p2p) from the average behaviour within the GroupID. Each letter can obtain the values A (highest quality), B, or C (lowest quality).
char
primary
filter_detection_flag
Number flag for the variability in this filter (0=non-variable, 1=variable).
char
primary
hcv_mean_mag
Mean of the light curve’s corrected magnitudes (if corrected, else the HSC).
mag
char
primary
hsc_mean_mag
Mean of the light curve’s HSC magnitudes.
mag
char
primary
mad
The median absolute deviation (MAD) of the magnitude.
char
primary
chi2
Value of the reduced χ² for the null-hypothesis of the source magnitude being constant.
char
primary
catalogues.mv_hipparcos_fdw
de_rad
Declination in ICRS, Ep=1991.25
radians
double
e_b_v
Formal error on colour index
mag
double
e_de_rad
Formal error on declination
mas
double
e_ra_rad
Formal error on right ascension
mas
double
f1
Percentage rejected data
int
f2
Goodness of fit
double
hip
Hipparcos identifier
int
ic
Entry in one of the suppl.catalogues
int
nc
Number of components
int
ntr
Number of field transits used
int
pos
Pgsphere point
spoint
char
ra_rad
Right Ascension in ICRS, Ep=1991.25
radians
double
s_hp
Scatter of Hipparcos magnitude
mag
double
sn
[0,159] Solution type new reduction
The solution type is a number 10xd+s consisting of two parts d and s:
- s describes the type of solution adopted:
1 = stochastic solution (dispersion is given in the 'var' column)
3 = VIM solution (additional parameters in file hipvim.dat)
5 = 5-parameter solution (this file)
7 = 7-parameter solution (additional parameters in hip7p.dat)
9 = 9-parameter solution (additional parameters in hip9p.dat)
- d describes peculiarities, as a combination of values:
0 = single star
1 = double star
2 = variable in the system with amplitude > 0.2mag
4 = astrometry refers to the photocenter
8 = measurements concern the secondary (fainter) in the double system
int
so
[0,5] Solution type old reduction
as follows:
0 = standard 5-parameter solution
1 = 7- or 9-parameter solution
2 = stochastic solution
3 = double and multiple stars
4 = orbital binary as resolved in the published catalog
5 = VIM (variability-induced mover) solution
int
u1
Upper-triangular weight matrix element 1
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u10
Upper-triangular weight matrix element 10
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u11
Upper-triangular weight matrix element 11
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u12
Upper-triangular weight matrix element 12
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u13
Upper-triangular weight matrix element 13
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u14
Upper-triangular weight matrix element 14
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u15
Upper-triangular weight matrix element 15
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u2
Upper-triangular weight matrix element 2
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u3
Upper-triangular weight matrix element 3
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u4
Upper-triangular weight matrix element 4
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u5
Upper-triangular weight matrix element 5
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u6
Upper-triangular weight matrix element 6
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u7
Upper-triangular weight matrix element 7
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u8
Upper-triangular weight matrix element 8
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
u9
Upper-triangular weight matrix element 9
The upper-triangular weight matrix U is related to the
covariance matrix C by
C-1 = ∼U U (∼U represents transposed U)
The elements Ui forming the upper triangular matrix are stored as
± -+
| (1) (2) (4) (7) (11) |
| 0 (3) (5) (8) (12) |
| 0 0 (6) (9) (13) |
| 0 0 0 (10) (14) |
| 0 0 0 0 (15) |
± -+
on the astrometric parameters RA, Dec, plx, pmRA, pmDE,
and derivatives of proper motions for 7- and 9-parameter
solutions.
double
va
Reference to variability annex
int
var
Cosmic dispersion added (stochastic solution)
double
name
Source name, Hipparcos identifier
meta.id;meta.main
char
primary
ra
Right Ascension in ICRS, Ep=1991.25
deg
pos.eq.ra;meta.main
double
primary
dec
Declination in ICRS, Ep=1991.25
deg
pos.eq.dec;meta.main
double
primary
plx
Parallax
mas
pos.parallax.trig
double
primary
e_plx
Formal error on plx
mas
double
primary
pm_ra
Proper motion in Right Ascension
mas/yr
pos.pm;pos.eq.ra
double
primary
e_pm_ra
Formal error on pm_ra
mas/yr
double
primary
pm_de
Proper motion in Declination
mas/yr
pos.pm;pos.eq.dec
double
primary
e_pm_de
Formal error on pm_de
mas/yr
double
primary
hp_mag
Hipparcos magnitude
mag
double
primary
e_hp_mag
Error on mean Hipparcos magnitude
mag
double
primary
b_v
Colour index
mag
double
primary
v_i
V-I colour index
mag
double
primary
catalogues.mv_lamost_dr8_lrs_fdw
postcard_url
meta.ref.url;meta.preview
char
primary
product_url
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
designation
char
primary
uid
char
gp_id
char
ra
Right Ascension from input catalog
pos.eq.ra;meta.main
double
primary
dec
Declination from input catalog
pos.eq.dec;meta.main
double
primary
obsid
Unique Spectra ID
int
primary
lmjd
Local Modified Julian Day
int
obsdate
Target Observation Date
char
primary
class
Stellar spectral type
char
primary
mjd
Modified Julian Day
int
planid
Plan Name
char
subclass
Stellar subclass
char
primary
spid
Spectrograph ID
degrees
double
z
Redshift
double
primary
fiberid
Fiber ID of object
degrees
double
z_err
Redshift uncertainty
double
primary
ra_obs
Right ascension of fiber pointing (J2000)
double
snru
Signal-to-noise ratio of u filter
double
primary
dec_obs
Declination of fiber pointing (J2000)
double
snrg
Signal-to-noise ratio of g filter
double
primary
snrr
Signal-to-noise ratio of r filter
double
primary
snri
Signal-to-noise ratio of i filter
double
primary
snrz
Signal-to-noise ratio of z filter
double
primary
ps_id
char
mag_ps_g
double
mag_ps_r
double
mag_ps_i
double
mag_ps_z
double
mag_ps_y
double
gaia_source_id
char
gaia_g_mean_mag
double
tsource
Organization or person who submit input catalog
char
fibertype
Fiber Type of target [Obj, Sky, F-std, Unused, PosErr, Dead]
char
tfrom
Input catalog submitted by an organization or a person determined by the tsource
char
tcomment
Target information
char
offsets
Whether there is a fiber offset during observation
boolean
offsets_v
If the ‘offsets’ field is true, ‘offsets_v’ gives the offset distance from the target’s coordinator in input catalog
double
fibermask
Fiber Mask
int
with_norm_flux
boolean
lamost_dr8_lrs_oid
meta.oid
int
npix
Healpix pixel of the center for nside 256
long
catalogues.mv_lamost_dr8_mrs_fdw
product_url
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
designation
char
primary
obsid
Unique Spectra ID
long
ra
Right Ascension from input catalog
degrees
pos.eq.ra;meta.main
double
primary
dec
Declination from input catalog
degrees
pos.eq.dec;meta.main
double
primary
uid
char
gp_id
char
mobsid
meta.id;meta.main
char
primary
obsdate
Target Observation Date
char
primary
band
Having two values of B and R, which represent B and R band spectra
char
primary
lmjd
Local Modified Julian Day
int
snr
The median value of all pixel S/Ns in B band spectrum or R band
double
primary
mjd
Modified Julian Day
int
rv_b0
double
primary
planid
Plan Name
char
rv_r0
double
primary
spid
Spectrograph ID
int
fiberid
Fiber ID of object
int
lmjm
Local modified Julian minute
int
ra_obs
Right ascension of fiber pointing (J2000)
double
dec_obs
Declination of fiber pointing (J2000)
double
gaia_source_id
char
gaia_g_mean_mag
double
gaia_bp_mean_mag
double
gaia_rp_mean_mag
double
tsource
Organization or person who submit input catalog
char
fibertype
Fiber Type of target [Obj, Sky, F-std, Unused, PosErr, Dead]
char
tfrom
Input catalog submitted by an organization or a person determined by the tsource
char
tcomment
Target information
char
offsets
Whether there is a fiber offset during observation
boolean
offsets_v
If the ‘offsets’ field is true, ‘offsets_v’ gives the offset distance from the target’s coordinator in input catalog
double
rv_b0_err
Uncertainty of rv_b0 measured by the method LASP used
double
rv_b1
Radial velocity after zero-point correction of rv_b0
double
rv_b1_err
Uncertainty of rv_b1 measured by the error propagation
double
rv_b_flag
Radial velocity flag for B band spectra
int
rv_r0_err
Uncertainty of rv_r0 measured by the method LASP used
double
rv_r1
Radial velocity after zero-point correction of rv_r0
double
rv_r1_err
Uncertainty of rv_r1 measured by the error propagation
double
rv_r_flag
Radial velocity flag for R band spectra
int
rv_br0
double
rv_br0_err
Uncertainty of rv_br0 measured by the method LASP used
double
rv_br1
Radial velocity after zero-point correction of rv_br0
double
rv_br1_err
Uncertainty of rv_br1 measured by the error propagation
double
rv_br_flag
Radial velocity flag for B and R band spectra
int
rv_lasp0
Radial velocity measured by the LASP
double
rv_lasp0_err
Uncertainty of rv_lasp0 also given by the LASP
double
rv_lasp1
Radial velocity after zero-point correction of rv_lasp0
double
rv_lasp1_err
Uncertainty of rv_lasp1 measured by the error propagation
double
coadd
A flag to show whether it is a coadd spectrum
boolean
fibermask
Possible fiber problems
int
bad_b
A flag to show whether the B band spectra is problematic
boolean
bad_r
A flag to show whether the R band spectra is problematic
boolean
moon_angle
The angular distance of each target to the moon
double
lunardate
The date of Chinese lunar canlendar, which represents the moon phase, and its value is from 1 to 30.
int
moon_flg
This is a flag for ‘moon_angle’, and it has two values of 0 and 1, which represent the range of angular distance. If ‘moon_flg’ equals to 1, it indicates that angular distance is in the range of [10 degree, 30 degree], and it represents that the angular distance is larger than 30 degree when ‘moon_flg’ equals to 0.
boolean
lamost_dr8_mrs_oid
meta.oid
int
npix
Healpix pixel of the center for nside 256
long
catalogues.mv_lamost_dr9_lrs_fdw
lamost_dr9_lrs_oid
null
meta.oid
int
postcard_url
meta.ref.url;meta.preview
char
primary
product_url
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
npix
Healpix pixel of the center of the observation for nside 256
long
obsid
Unique Spectra ID
meta.id
int
primary
uid
Unique source identifier calculated with the "ura" and "udec" in table 10
meta.id;meta.main
char
gp_id
For each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 10) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.
meta.id.assoc
long
designation
Target designation
meta.id
char
primary
obsdate
Target Observation Date
meta.ref;time.epoch
char
primary
lmjd
Local modified Julian day
d
meta.ref;time.epoch
int
mjd
Modified Julian Day
d
meta.ref;time.epoch
int
planid
Plan Name
meta.code
char
spid
Spectrograph ID
meta.id
short
fiberid
Fiber ID of object
meta.id.assoc
short
ra_obs
Fiber pointing right ascension
deg
pos.eq.ra
double
dec_obs
Fiber pointing declination
deg
pos.eq.dec
double
snru
Signal-to-noise ratio of u filter
stat.snr;phot.flux;em.opt.U
double
primary
snrg
Signal-to-noise ratio of g filter
stat.snr;phot.flux;em.opt.V
double
primary
snrr
Signal-to-noise ratio of r filter
stat.snr;phot.flux;em.opt.R
double
primary
snri
Signal-to-noise ratio of i filter
stat.snr;phot.flux;em.opt.I
double
primary
snrz
Signal-to-noise ratio of z filter
stat.snr;phot.flux;em.opt.I
double
primary
class
Spectral type
meta.code.class
char
primary
subclass
Stellar spectral type
src.spType
char
primary
z
Redshift
src.redshift
double
primary
z_err
Redshift uncertainty
stat.error;src.redshift
double
primary
ps_id
The objID in the Pan-STARRS catalog
meta.id.assoc
long
mag_ps_g
Pan-STARRS g band magnitude
phot.flux;em.opt.V
double
mag_ps_r
Pan-STARRS r band magnitude
mag
phot.flux;em.opt.R
double
mag_ps_i
Pan-STARRS i band magnitude
mag
phot.flux;em.opt.I
double
mag_ps_z
Pan-STARRS z band magnitude
mag
phot.flux;em.opt.I
double
mag_ps_y
Pan-STARRS y band magnitude
mag
phot.flux;em.opt.I
double
gaia_source_id
The "source_id" field of Gaia DR3 catalog
meta.id.assoc
char
gaia_g_mean_mag
The "phot_g_mean_magnitude" field of Gaia DR3 catalog
mag
phot.mag;em.opt
double
fibertype
Fiber Type of target [Obj, Sky, F-std, Unused, PosErr, Dead]
meta.code.class
char
offsets
Whether there is a fiber offset during observation
meta.code.class
short
offsets_v
If the “offsets” field is true, “offsets_v” gives the offset distance from the target’s coordinator in input catalog
arcsec
instr.offset
double
ra
Right Ascension from input catalog
deg
pos.eq.ra;meta.main
double
primary
dec
Declination from input catalog
deg
pos.eq.dec;meta.main
double
primary
fibermask
Possible fiber problems
meta.code
short
with_norm_flux
It has two values of 0 and 1, 1 represents the FITS file provides the normalized spectrum, and 0 means it does not. The normalized flux is in the data array of extension 1.
meta.code
short
catalogues.mv_lamost_dr9_mrs_fdw
lamost_dr9_mrs_oid
null
meta.oid
int
product_url
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
npix
Healpix pixel of the center of the observation for nside 256
long
mobsid
Unique ID for each medium-resolution spectrum in each exposure
meta.id.assoc;meta.main
char
primary
obsid
Unique spectrum ID for each observation of each target
meta.id
int
uid
Unique source identifier calculated with the "ura" and "udec" in table 9
meta.id
char
gp_id
For each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey ((Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.
meta.id
long
designation
Target designation
meta.id
char
primary
obsdate
Target Observation Date
meta.ref;time.epoch
char
primary
lmjd
Local Modified Julian Day
d
meta.ref;time.epoch
int
mjd
Modified Julian Day
d
meta.ref;time.epoch
int
planid
Plan Name
meta.code
char
spid
Spectrograph ID
meta.id
short
fiberid
Fiber ID
meta.id.assoc
short
lmjm
Local modified Julian minute
min
meta.ref;time.epoch
int
band
Having two values of B and R, which represent B and R band spectra
instr.bandpass
char
primary
ra_obs
Fiber pointing right ascension
deg
pos.eq.ra
double
dec_obs
Fiber pointing declination
deg
pos.eq.dec
double
snr
The median value of all pixel S/Ns in B band spectrum or R band
stat.snr
double
primary
gaia_source_id
The "source_id" field of Gaia DR3 catalog
meta.id.assoc
char
gaia_g_mean_mag
The "phot_g_mean_mag" field of Gaia DR3 catalog
mag
phot.mag;em.opt
double
gaia_bp_mean_mag
The "phot_bp_mean_mag" field of Gaia DR3 catalog
mag
phot.mag;em.opt.B
double
gaia_rp_mean_mag
The "phot_rp_mean_mag" field of Gaia DR3 catalog
mag
phot.mag;em.opt.R
double
fibertype
Fiber Type of target [Obj, Sky, F-std, Unused, PosErr, Dead]
meta.code.class
char
offsets
Whether there is a fiber offset during observation
meta.code.class
short
offsets_v
If the “offsets” field is true, “offsets_v” gives the offset distance from the targets coordinator in input catalog
arcsec
instr.offset
double
ra
Right Ascension from input catalog
deg
pos.eq.ra;meta.main
double
primary
dec
Declination from input catalog
deg
pos.eq.dec;meta.main
double
primary
rv_b0
Radial velocity of B band spectra measured with 483 selected KURUCZ synthetic templates
km/s
spect.dopplerVeloc.opt;em.opt.B
double
primary
rv_b0_err
Uncertainty of rv_b0 measured by the method LASP used
km/s
stat.error;spect.dopplerVeloc.opt;em.opt.B
double
rv_b1
Radial velocity after zero-point correction of rv_b0
km/s
spect.dopplerVeloc.opt;em.opt.B
double
rv_b1_err
Uncertainty of rv_b1 measured by the error propagation
km/s
stat.error;spect.dopplerVeloc.opt;em.opt.B
double
rv_b_flag
Radial velocity flag for B band spectra
meta.code.class
short
rv_r0
Radial velocity of R band spectra measured with 483 selected KURUCZ synthetic templates
km/s
spect.dopplerVeloc.opt;em.opt.R
double
primary
rv_r0_err
Uncertainty of rv_r0 measured by the method LASP used
km/s
stat.error;spect.dopplerVeloc.opt;em.opt.R
double
rv_r1
Radial velocity after zero-point correction of rv_r0
km/s
spect.dopplerVeloc.opt;em.opt.R
double
rv_r1_err
Uncertainty of rv_r1 measured by the error propagation
km/s
stat.error;spect.dopplerVeloc.opt;em.opt.R
double
rv_r_flag
Radial velocity flag for R band spectra
meta.code.class
short
rv_br0
Radial velocity of B and R band spectra measured with 483 selected KURUCZ synthetic templates
km/s
spect.dopplerVeloc.opt;em.opt
double
rv_br0_err
Uncertainty of rv_br0 measured by the method LASP used
km/s
stat.error;spect.dopplerVeloc.opt;em.opt
double
rv_br1
Radial velocity after zero-point correction of rv_br0
km/s
spect.dopplerVeloc.opt;em.opt
double
rv_br1_err
Uncertainty of rv_br1 measured by the error propagation
km/s
stat.error;spect.dopplerVeloc.opt;em.opt
double
rv_br_flag
Radial velocity flag for B and R band spectra
meta.code.class
short
rv_lasp0
Radial velocity measured by the LASP
km/s
spect.dopplerVeloc.opt;em.opt
double
rv_lasp0_err
Uncertainty of rv_lasp0 also given by the LASP
km/s
stat.error;spect.dopplerVeloc.opt;em.opt
double
rv_lasp1
Radial velocity after zero-point correction of rv_lasp0
km/s
spect.dopplerVeloc.opt;em.opt
double
rv_lasp1_err
Uncertainty of rv_lasp1 measured by the error propagation
km/s
stat.error;spect.dopplerVeloc.opt;em.opt
double
coadd
A flag to show whether it is a coadd spectrum
meta.code.class
short
fibermask
Possible fiber problems
meta.code
short
bad_b
A flag to show whether the B band spectra is problematic
meta.code.class
short
bad_r
A flag to show whether the R band spectra is problematic
meta.code.class
short
moon_angle
The angular distance of each target to the moon
deg
pos.angDistance
double
lunardate
The date of Chinese lunar canlendar, which represents the moon phase, and its value is from 1 to 30.
meta.ref;time.epoch
short
moon_flg
This is a flag for “moon_angle”, and it has two values of 0 and 1, which represent the range of angular distance. If “moon_flg” equals to 1, it indicates that angular distance is in the range of [10 degree, 30 degree], and it represents that the angular distance is larger than 30 degree when “moon_flg” equals to 0.
meta.code.class
char
subproject
The sub-project names of LAMOST Medium-Resolution Spectroscopic Survey
meta.code.class
char
catalogues.mv_ou4blazars_fdw
id
int
npix
long
original_catalog
Original catalogue from which the source was taken
char
ou4blazars_oid
int
source_name
Source designation
meta.id;meta.main
char
primary
ra
Source R.A. (J2000.0)
degrees
pos.eq.ra;meta.main
double
primary
dec
Source Dec. (J2000.0)
degrees
pos.eq.dec;meta.main
double
primary
radio_flux
Radio flux density at 1.4 or 0.8 GHz (mJy)
mag
double
primary
fermi_flux
Fermi 8yr photon flux E > 1GeV
mag
double
primary
log_nu_peak
Log of synchrotron peak frequency (Hz)
double
primary
redshift
Source redshift
double
primary
catalogues.mv_pcss_catalog_excluded_fdw
highest_reliability_cat
The highest reliability catalogue to which the source belongs. As the full catalogue reliability is >=80%, this is the lowest possible value in this column.
int
pos
pgsphere spoint representation of the position (ra, dec)
radians
char
name
Name of source
meta.id;meta.main
char
primary
ra
Right ascension of source (J2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination of source (J2000)
deg
pos.eq.dec;meta.main
double
primary
frequency
Planck Frequency
GHz
int
primary
detflux
Flux density of source as determined by detection method
mJy
float
primary
detflux_err
Uncertainty (1 sigma) in channel flux density
mJy
float
primary
extended
Extended source flag, 0 if the source is compact and 1 if the source is extended.
int
primary
catalogues.mv_pcss_catalog_hfi_fdw
pos
pgsphere spoint representation of the position (ra, dec)
radians
char
name
Name of source
meta.id;meta.main
char
primary
ra
Right ascension of source (J2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination of source (J2000)
deg
pos.eq.dec;meta.main
double
primary
frequency
Planck Frequency
GHz
int
primary
detflux
Channel flux density
mJy
float
primary
detflux_err
Error (1 sigma) in channel flux density
mJy
float
primary
extended
Extended source flag, 0 if the source is compact and 1 if the source is extended.
int
primary
highest_reliability_cat
The highest reliability catalogue to which the source belongs. As the full catalogue reliability is >=80%, this is the lowest possible value in this column.
int
primary
catalogues.mv_pcss_catalog_lfi_fdw
pos
pgsphere spoint representation of the position (ra, dec)
radians
char
name
Name of source
meta.id;meta.main
char
primary
ra
Right ascension of source (J2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination of source (J2000)
deg
pos.eq.dec;meta.main
double
primary
frequency
Planck Frequency
GHz
int
primary
detflux
Channel flux density
mJy
float
primary
detflux_err
Error (1 sigma) in channel flux density
mJy
float
primary
extended
Extended source flag, 0 if the source is compact and 1 if the source is extended.
int
primary
highest_reliability_cat
The highest reliability catalogue to which the source belongs. As the full catalogue reliability is >=80%, this is the lowest possible value in this column.
int
primary
catalogues.mv_plato_pic_target_go_fdw
PICname
char
"RAdeg"
pos.eq.ra;meta.main
double
"DEdeg"
pos.eq.dec;meta.main
double
active_end_date
char
active_start_date
char
"AG"
double
"AKs"
double
"BOLnCameraObsNCAM_T"
int
"BOLnCameraSatNCAM_T"
int
"BOLrandomNSRNCAM_T"
double
"BOLrandomSysNSRNCAM_T"
double
"BPmag"
double
"caseFlag"
int
"cPICsourceFlag"
int
"distance"
double
"eAG"
double
"eAKs"
double
"eBPmag"
double
"EBPRP"
double
"eDEdeg"
double
edistance
double
"eEBPRP"
double
"eGmag"
double
"eHpmag"
double
"eKsmag"
double
"eMass"
double
"EOLnCameraObsNCAM_R"
int
"EOLnCameraSatNCAM_R"
int
"EOLrandomNSRNCAM_R"
double
"EOLrandomSysNSRNCAM_R"
double
"ePlatoMagFCAMb"
double
"ePlatoMagFCAMr"
double
"ePlatoMagNCAM"
double
"ePlx"
double
epm
double
"epmDE"
double
"epmRA"
double
"eRAdeg"
double
"eRadius"
double
"eRPmag"
double
"eTeff"
double
"eVmagCalculated"
double
"extStatus"
int
"fgPICcPICvariabilityFlag"
int
"fgPICsourceFlag"
int
"Glat"
double
"Glon"
double
"Gmag"
double
"Hpmag"
double
"Ksmag"
double
"Mass"
double
mission_configuration_id
long
npix
long
"NSSFlag"
int
"PICid"
long
"PICmainSourceFlagBOL"
int
pic_target_go_oid
int
"PlatoMagFCAMb"
double
"PlatoMagFCAMr"
double
"PlatoMagNCAM"
double
"Plx"
double
pm
double
"pmDE"
double
"pmRA"
double
"posEpoch"
double
"posPropFlag"
int
"qualityFlag"
int
"Radius"
double
"refEpoch"
double
"RPmag"
double
"scheduledTarget"
int
"scientificPriority"
int
"scvPICscientificRanking"
int
"scvPICsourceFlag"
int
StarName
char
"targetStatusFlag"
int
"Teff"
double
"tPICplanetFlag"
int
"tPICscientificRanking"
double
"tPICsourceFlagNCAM_BOL"
int
"VmagCalculated"
double
catalogues.mv_t_chandra_csc2_fdw
name
Name of source
meta.id;meta.main
char
primary
ra
Right ascension of source (J2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination of source (J2000)
deg
pos.eq.dec;meta.main
double
primary
flux_aper_b
ACIS broad band, b (0.5-7.0 keV), aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events
erg·cm-2·s-1
double
primary
flux_aper_lolim_b
Lower 1 sigma (68.2%) Flux ACIS broad band, b (0.5-7.0 keV) confidence limit
erg·cm-2·s-1
double
primary
flux_aper_hilim_b
Upper 1 sigma (68.2%) Flux ACIS broad band, b (0.5-7.0 keV) confidence limit
erg·cm-2·s-1
double
primary
flux_aper_w
HRC wide band, w (~0.1-10.0 keV), aperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events
erg·cm-2·s-1
double
primary
flux_aper_lolim_w
Lower 1 sigma (68.2%) Flux HRC wide band, w (~0.1-10.0 keV), confidence limit
erg·cm-2·s-1
double
primary
flux_aper_hilim_w
Upper 1 sigma (68.2%) Flux HRC wide band, w (~0.1-10.0 keV), confidence limit
erg·cm-2·s-1
double
primary
flux_aper_avg_b
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band
erg·cm-2·s-1
double
primary
flux_aper_avg_lolim_b
Lower 1 sigma (68.2%) average Flux ACIS broad band, b (0.5-7.0 keV), confidence limit
erg·cm-2·s-1
double
primary
flux_aper_avg_hilim_b
Upper 1 sigma (68.2%) average Flux ACIS broad band, b (0.5-7.0 keV), confidence limit
erg·cm-2·s-1
double
primary
flux_aper_avg_w
Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy band
erg·cm-2·s-1
double
primary
flux_aper_avg_lolim_w
Lower 1 sigma (68.2%) average Flux HRC wide band, w (~0.1-10.0 keV), confidence limit
erg·cm-2·s-1
double
primary
flux_aper_avg_hilim_w
Upper 1 sigma (68.2%) average Flux HRC wide band, w (~0.1-10.0 keV), confidence limit
erg·cm-2·s-1
double
primary
err_ellipse_r0
Major radius of the 95% confidence level position error ellipse
arcsec
double
primary
err_ellipse_r1
Minor radius of the 95% confidence level position error ellipse
arcsec
double
primary
err_ellipse_ang
Position angle (referenced from local true north) of the major axis of the 95% confidence level error ellipse
deg
double
primary
significance
Highest flux significance across all stacked observations and science energy bands
double
primary
likelihood
Highest detection log-likelihood across all stacked observations and science energy bands
double
primary
likelihood_class
Highest detection likelihood classification across all stacked observations and science energy bands
char
primary
conf_flag
Source may be confused (source and/or background regions overlap in one or more contributing stacked observations)
int
primary
extent_flag
Source is extended, or deconvolved source extent is inconsistent with a point source at the 90% confidence level in one or more observations and science energy bands
int
primary
sat_src_flag
Source is saturated in all observations; source properties are unreliable
int
primary
streak_src_flag
Source is located on an ACIS readout streak in all observations; source properties may be affected
int
primary
var_flag
Source displays flux variability within one or more observations, or between observations, in one or more energy bands
int
primary
var_inter_hard_flag
Source hardness ratios are statistically inconsistent between two or more observations
int
primary
hard_hm
ACIS hard (2.0-7.0 keV) - medium (1.2-2.0 keV) energy band hardness ratio
double
primary
hard_hm_lolim
ACIS hard (2.0-7.0 keV) - medium (1.2-2.0 keV) energy band hardness ratio (68% lower confidence limit)
double
primary
hard_hm_hilim
ACIS hard (2.0-7.0 keV) - medium (1.2-2.0 keV) energy band hardness ratio (68% upper confidence limit)
double
primary
hard_ms
ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio
double
primary
hard_ms_lolim
ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)
double
primary
hard_ms_hilim
ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)
double
primary
var_intra_index_b
Intra-observation Gregory-Loredo variability index in the range [0, 10] for the ACIS broad band, b (0.5-7.0 keV). A low value indicates that the source region photon flux is constant between observations whereas a high value indicates that the source is very likely to be variable
int
primary
var_intra_index_w
Intra-observation Gregory-Loredo variability index in the range [0, 10] for the wide band, w (~0.1-10.0 keV). A low value indicates that the source region photon flux is constant within an observation (highest value across all observations), whereas a high value indicate that flux is variable within the observation
int
primary
var_inter_index_b
Inter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations for the broad band, b (0.5-7.0 keV)
int
primary
var_inter_index_w
Inter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations for the wide band, w (~0.1-10.0 keV)
int
primary
var_inter_hard_prob_hm
Inter-observation ACIS hard (2.0-7.0 keV) - medium (1.2-2.0 keV) energy band hardness ratio variability probability, which indicates whether the source is spectrally variable when these two bands are considered
double
primary
var_inter_hard_prob_ms
Inter-observation ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio variability probability, which indicates whether the source is spectrally variable when these two bands are considered
double
primary
acis_time
Total livetime for all ACIS imaging observations contributing to the Master Sources Table record of the source
seconds
double
primary
hrc_time
Total livetime for all HRC imaging observations contributing to the Master Sources Table record of the source
seconds
double
primary
catalogues.mv_t_hubble_scv3_fdw
abs_corr
Y/N indicator of whether the astrometric correction included alignment with a standard catalog
char
ci
Normalized (by detector and filter) mean value of Concentration Index, defined as difference between magnitude in small and large apertures
double
ci_sigma
Std dev in measurements of normalized Concentration Index
double
dsigma
Std dev of source positions and match position
milliarcseconds
double
extinction
E(B-V) from Schlegel et al. (1998)
ABMag
double
htmid
Hierarchical triangular index (HTM) identifier
long
kron_radius
Mean value of the Kron Radius from Source Extractor
arcseconds
double
kron_radius_sigma
Std dev in measurements of Kron Radius
arcseconds
double
num_filters
Number of filters used in the match
int
num_visits
Number of visits used in the match
int
spectrum_flag
Indicates spectrum is available
char
start_mjd
Observation Start Time (Mean Julian Date - MJD) for earliest observation in match
MJD
double
start_time
Observation Start Time for earliest observation in match
time
time.start
char
stop_mjd
Observation Stop Time for latest observation in match
MJD
double
stop_time
Observation Stop Time for latest observation in match
time
char
x
x coordinate of source on unit celestial sphere
double
y
y coordinate of source on unit celestial sphere
double
z
z coordinate of source on unit celestial sphere
double
match_id
The HSC match ID number.
meta.id;meta.main
long
primary
target_name
Target name for one of the observations
char
primary
num_images
Number of images used in the match
int
primary
num_images_per_filter
Number of images per filter
int
primary
ra
Right ascension for the match (J2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination for the match (J2000)
deg
pos.eq.dec;meta.main
double
primary
filter
Filter for the match, one filter per row. First part of the filter name corresponds to the instrument, where w3 = WPC3; w2 = WFPC2; a = ACS
char
primary
flux
Median magnitude for the corresponding filter
mag
double
primary
flux_sigma
Median absolute deviation around the median magnitude
mag
double
primary
catalogues.mv_tycho2_fdw
ccdm
CCDM component identifier for HIP stars. The CCDM component identifiers for double or multiple Hipparcos stars contributing to this Tycho-2 entry. For photocentre solutions, all components within 0.8 arcsec contribute. For double star solutions any unresolved component within 0.8 arcsec contributes. For single star solutions, the predicted signal from close stars were normally subtracted in the analysis of the photon counts and such stars therefore do not contribute to the solution. The components are given in lexical order.
char
corr
Correlation (ra_deg, de_deg)
double
de_deg
Observed Tycho-2 Declination, ICRS
deg
double
de_mdeg
Mean Declination, ICRS, at epoch=J2000 The mean position is a weighted mean for the catalogues contributing to the proper motion determination. This mean has then been brought to epoch 2000.0 by the computed proper motion. See Note(2) above for details. Tycho-2 is one of the several catalogues used to determine the mean position and proper motion. The observed Tycho-2 position is given in the fields ra_deg and de_deg.
deg
double
e_de_deg
Statistical error of observed Tycho-2 Dec. The errors are based on error models.
mas
double
e_de_mdeg
Statistical error of Dec at mean epoch. The errors are based on error models.
mas
double
ep_de1990
Epoch-1990 of de_deg
yr
float
ep_de_m
Mean epoch of Dec. The mean epochs are given in Julian years.
yr
meta.ref;time.epoch
float
ep_ra1990
Epoch-1990 of ra_deg
yr
float
ep_ra_m
Mean epoch of RA. The mean epochs are given in Julian years.
yr
meta.ref;time.epoch
float
e_ra_deg
Statistical error RA*cos(dec), of observed Tycho-2 RA. The errors are based on error models.
mas
double
e_ra_mdeg
Statistical error RA*cos(dec),at mean epoch. The errors are based on error models.
mas
double
id_tycho
(TYC1,TYC2 and TYC3) are combined into one complete number given by (TYC1*1000000.0d0)+(TYC2*10.0d0)+(TYC3*1.0d0).
long
num
Number of positions used
short
pflag
Mean position flag. ' ' = normal mean position and proper motion. 'P' = the mean position, proper motion, etc., refer to the photocentre of two Tycho-2 entries, where the BT magnitudes were used in weighting the positions. 'X' = no mean position, no proper motion.
char
pos
char
posflg
Type of Tycho-2 solution. ' ' = normal treatment, close stars were subtracted when possible. 'D' = double star treatment. Two stars were found. The companion is normally included as a separate Tycho-2 entry, but may have been rejected. 'P' = photocentre treatment, close stars were not subtracted. This special treatment was applied to known or suspected doubles which were not successfully (or reliably) resolved in the Tycho-2 double star processing.
char
prox
Proximity indicator. Distance in units of 100 mas to the nearest entry in the Tycho-2 main catalogue or supplement. The distance is computed for the epoch 1991.25. A value of 999 (i.e. 99.9 arcsec) is given if the distance exceeds 99.9 arcsec.
100mas
short
q_de_mdeg
Goodness of fit for mean Dec. This goodness of fit is the ratio of the scatter-based and the model-based error. It is only defined when Num > 2. Values exceeding 9.9 are truncated to 9.9.
float
q_pm_de
Goodness of fit for pm_de. This goodness of fit is the ratio of the scatter-based and the model-based error. It is only defined when Num > 2. Values exceeding 9.9 are truncated to 9.9.
float
q_pm_ra
Goodness of fit for pm_ra. This goodness of fit is the ratio of the scatter-based and the model-based error. It is only defined when Num > 2. Values exceeding 9.9 are truncated to 9.9.
float
q_ra_mdeg
Goodness of fit for mean RA. This goodness of fit is the ratio of the scatter-based and the model-based error. It is only defined when Num > 2. Values exceeding 9.9 are truncated to 9.9.
float
ra_deg
Observed Tycho-2 Right Ascension, ICRS
deg
pos.eq.ra;meta.main
double
ra_mdeg
Mean Right ascension, ICRS, epoch=J2000. The mean position is a weighted mean for the catalogues contributing to the proper motion determination. This mean has then been brought to epoch 2000.0 by the computed proper motion. See Note(2) above for details. Tycho-2 is one of the several catalogues used to determine the mean position and proper motion. The observed Tycho-2 position is given in the fields ra_deg and de_deg.
deg
double
tyc
Tycho-1 star. ' ' = no Tycho-1 star was found within 0.8 arcsec (quality 1-8) or 2.4 arcsec (quality 9). 'T' = this is a Tycho-1 star. The Tycho-1 identifier is given in the beginning of the record. For Tycho-1 stars, resolved in Tycho-2 as a close pair, both components are flagged as a Tycho-1 star and the Tycho-1 TYC3 is assigned to the brightest (VT) component. The HIP-only stars given in Tycho-1 are not flagged as Tycho-1 stars.
char
tyc1
TYC1 from TYC or GSC. The TYC identifier is constructed from the GSC region number (TYC1), the running number within the region (TYC2) and a component identifier (TYC3) which is normally 1. Some non-GSC running numbers were constructed for the first Tycho Catalogue and for Tycho-2. The recommended star designation contains a hyphen between the TYC numbers, e.g. TYC 1-13-1.
char
tyc2
TYC2 from TYC or GSC. The TYC identifier is constructed from the GSC region number (TYC1), the running number within the region (TYC2) and a component identifier (TYC3) which is normally 1. Some non-GSC running numbers were constructed for the first Tycho Catalogue and for Tycho-2. The recommended star designation contains a hyphen between the TYC numbers, e.g. TYC 1-13-1.
char
tyc3
TYC3 from TYC. The TYC identifier is constructed from the GSC region number (TYC1), the running number within the region (TYC2) and a component identifier (TYC3) which is normally 1. Some non-GSC running numbers were constructed for the first Tycho Catalogue and for Tycho-2. The recommended star designation contains a hyphen between the TYC numbers, e.g. TYC 1-13-1.
char
name
The Tycho 2 identifier (without the TYC letters at the start of the name). The TYC identifier is constructed from the GSC region number (TYC1), the running number within the region (TYC2) and a component identifier (TYC3) which is normally 1. Some non-GSC running numbers were constructed for the first Tycho Catalogue and for Tycho-2. The recommended star designation contains a hyphen between the TYC numbers, e.g. TYC 1-13-1.
meta.id;meta.main
char
primary
ra
Observed Tycho-2 Right Ascension, ICRS
deg
pos.eq.ra;meta.main
double
primary
dec
Observed Tycho-2 Declination, ICRS
deg
pos.eq.dec;meta.main
double
primary
pm_ra
Proper motion in RA*cos(dec). Some Hipparcos stars (having a positive number in the HIP column) have no proper motions; these are virtually all in multiple systems.
mas/yr
pos.pm;pos.eq.ra
float
primary
e_pm_ra
Statistical error of proper motion in RA*cos(dec). The errors are based on error models.
mas/yr
float
primary
pm_de
Proper motion in Declination. Some Hipparcos stars (having a positive number in the HIP column) have no proper motions; these are virtually all in multiple systems.
mas/yr
pos.pm;pos.eq.dec
float
primary
e_pm_de
Statistical error of proper motion in Dec. The errors are based on error models.
mas/yr
float
primary
bt_mag
Tycho-2 BT magnitude. Blank when no magnitude is available. Either bt_mag or vt_mag is always given. Approximate Johnson photometry may be obtained as: V = VT -0.090*(BT-VT); B-V = 0.850*(BT-VT). Consult Sect 1.3 of Vol 1 of "The Hipparcos and Tycho Catalogues", ESA SP-1200, 1997, for details.
mag
float
primary
e_bt_mag
Statistical error of BT. Blank when no magnitude is available. Either bt_mag or vt_mag is always given. Approximate Johnson photometry may be obtained as: V = VT -0.090*(BT-VT); B-V = 0.850*(BT-VT). Consult Sect 1.3 of Vol 1 of "The Hipparcos and Tycho Catalogues", ESA SP-1200, 1997, for details.
mag
float
primary
vt_mag
Tycho-2 VT magnitude. Blank when no magnitude is available. Either bt_mag or vt_mag is always given. Approximate Johnson photometry may be obtained as: V = VT -0.090*(BT-VT); B-V = 0.850*(BT-VT). Consult Sect 1.3 of Vol 1 of "The Hipparcos and Tycho Catalogues", ESA SP-1200, 1997, for details.
mag
float
primary
e_vt_mag
Statistical error of VT. Blank when no magnitude is available. Either bt_mag or vt_mag is always given. Approximate Johnson photometry may be obtained as: V = VT -0.090*(BT-VT); B-V = 0.850*(BT-VT). Consult Sect 1.3 of Vol 1 of "The Hipparcos and Tycho Catalogues", ESA SP-1200, 1997, for details.
mag
float
primary
hip
Hipparcos number
char
primary
catalogues.mv_v_gcc_catalog_fdw
pos
pgsphere spoint representation of the position (ra, dec)
radians
char
name
Source Name
meta.id;meta.main
char
primary
ra
Right ascension (J2000) in degrees
deg
pos.eq.ra;meta.main
double
primary
dec
Declination (J2000) in degrees
deg
pos.eq.dec;meta.main
double
primary
snr
Maximum S/N over the 857, 545, and 353GHz Planck cold residual maps
float
primary
gau_major_axis
FWHM along the major axis of the elliptical Gaussian
arcmin
float
primary
gau_major_axis_sig
1-sigma uncertainty on FWHM along the major axis
arcmin
float
primary
gau_minor_axis
FWHM along the minor axis of the elliptical Gaussian
arcmin
float
primary
gau_minor_axis_sig
1-sigma uncertainty on FWHM along the minor axis
arcmin
float
primary
catalogues.mv_v_hsa_cat_hppsc_070_fdw
band
This is one of the strings "blue","green","red" identifying the PACS detector array names for the filter bands centred at 70, 100, 160 microns, respectively. The wavelength is also specified in the name of the object.
microns
char
decerr
Positional uncertainties of each object as provided by SUSSEXtractor. Units are degrees, the data type is double precision.
deg
double
fratio
The ratio of the flux density values measured in the 6th and the 1st aperture, corresponding to 4?? and 9?? in the blue and green bands, and 9?? and 14?? in the red band.
double
raerr
Positional uncertainties of each object as provided by SUSSEXtractor. Units are degrees, the data type is double precision.
deg
double
snrnoise
It is calculated from the source flux and the estimated S/Ns, by dividing the flux by the S/Ns. This noise includes both the sky confusion and the instrument noise.
double
strn
Structure noise value obtained from the structure noise maps. Double precision, in units of MJy/sr.
MJy/sr
double
name
The object name is an identifier consisting of two parts, acronym and sequence, and is formatted as ’HPPSCxxxA_Jhhmmss.s±ddmmss’. ’HPPSC’ stands for Herschel PACS Point Source Catalogue, xxx is the central wavelength of the band in which the source was observed, identifying the wavelength in microns, and the letter A indicates the first version of the catalogue. The second part has the format ’Jhhmmss.s+ddmmss’ derived from the source coordinates with ’J’ indicating a J2000 reference system, ’hhmmss.s’ is the Right Ascension in hours, minutes and seconds accuracy of one digits after the decimal, and ’+ddmmss’ is the Declination in signed degrees, minutes and seconds to an accuracy of one digit after the decimal.
meta.id;meta.main
char
primary
ra
Right Ascension coordinate in a J2000.0 reference frame. This is the peak position of the SUSSEXtractor detection. The coordinates are degrees written in double precision format.
deg
pos.eq.ra;meta.main
double
primary
dec
Declination coordinate in a J2000.0 reference frame. This is the peak position of the SUSSEXtractor detection. The coordinates are degrees written in double precision format.
deg
pos.eq.dec;meta.main
double
primary
flux
This is the flux as provided by the AnnularSkyAperturePhotometry task. For objects that were identified several times across different maps, this flux corresponds to the extraction with the best average S/N, where the Ns based S/N (S/Ns)and the background RMS based S/N (S/Nr) values are taken into account. For the blue and green bands the aperture radius was 6??, for the red band 12?? (see Section 3.3 for more details). For all cases the raw flux density values were corrected for the aperture size, based on Lutz (2015). Colour corrections were not applied. The units are mJy, written as double precision.
mJy
double
primary
rms
RMS noise as measured in the blank sky apertures placed around the source. Double precision.
mJy
double
primary
fwhmxfit
FWHM in x direction. This column contains the FWHM values measured by the 2D Gaussian model in X and Y directions, fitted by the sourceFitter() task. If the elongated Gaussian fit was possible then both FWHMx and FWHMy are listed. If only a circular Gaussian could be fitted then FWHMy is equal to -99.9. It is written in double precision format, in units of second of arc.
arcseconds
double
primary
fwhmyfit
FWHM in y direction. This column contains the FWHM values measured by the 2D Gaussian model in X and Y directions, fitted by the sourceFitter() task. If the elongated Gaussian fit was possible then both FWHMx and FWHMy are listed. If only a circular Gaussian could be fitted then FWHMy is equal to -99.9. It is written in double precision format, in units of second of arc.
arcseconds
double
primary
snr
Estimated S/N based on a statistical approach, using the S/Ns calibration surfaces. It is calculated as a function of the source flux and the Ns value. The data type is double precision.
double
primary
stn
Calculated as the ratio of the source flux and the RMS. Data type is double precision.
double
primary
elong_flag
If an elliptical Gaussian model was fitted in the source, this column contains the ratio of the FWHMy and FWHMx. A value of 0 means that the source is circular, 0.5 means that FWHMy = 0.5 × FWHMx. If FWHMy = -99.9 (circular detection), FLAG_ELONG = 0. FLAG_ELONG is also set to 0 if the source eccentricity (FWHMx - FWHMy)/FWHMx) defined in a similar way with the FWHM values of the PACS PSF reported in Table 1, is smaller than the PSF eccentricity, Double precision format.
double
primary
edge_flag
The position of a source with respect to the edges of the image affects the quality of the photometry, as the extraction procedure needs a large enough area to compute properly both the flux density and the background to be subtracted. Also, due to the scan speed inhomogeneities during the turnarounds, the map edges may have different noise properties than the rest of the image.
boolean
primary
blend_flag
Objects with distance within the PSF FWHM have the same value (>0) of FLAG_BLEND and they can be considered as blended sources. FLAG_BLEND = 0 means that the object is not blended with other objects. The PACS PSFs depend on the observing mode. The absolute pointing error for SPG13 (1.2??) is adopted as uncertainty.
double
primary
warmat
Flag indicating that the observation was affected by "warm" attitude. The term refers to spacecraft attitudes in which the star-tracker support structure is subject to thermal distortions as was not completely shaded from sunlight. This has an impact on the pointing accuracy. Data type is Boolean.
boolean
primary
ssomap_flag
Maps of solar system objects have typically been observed in tracking mode, but were reprocessed in the ’rest’ sky frame for the HPPSC, and may be contaminated by the moving targets. The affected OBSIDs are marked with an ’ssomap’ flag.
boolean
primary
obsid
The term is the observation identifier for the Herschel observations . It is a 10 digit integer, starting always with 1342. The column lists the first OBSID from the list that built the L2.5/L3 map. It corresponds to the meta keyword obsid001.
char
primary
catalogues.mv_v_hsa_cat_hppsc_100_fdw
band
This is one of the strings "blue","green","red" identifying the PACS detector array names for the filter bands centred at 70, 100, 160 microns, respectively. The wavelength is also specified in the name of the object.
microns
char
decerr
Positional uncertainties of each object as provided by SUSSEXtractor. Units are degrees, the data type is double precision.
deg
double
fratio
The ratio of the flux density values measured in the 6th and the 1st aperture, corresponding to 4?? and 9?? in the blue and green bands, and 9?? and 14?? in the red band.
double
raerr
Positional uncertainties of each object as provided by SUSSEXtractor. Units are degrees, the data type is double precision.
deg
double
snrnoise
It is calculated from the source flux and the estimated S/Ns, by dividing the flux by the S/Ns. This noise includes both the sky confusion and the instrument noise.
double
strn
Structure noise value obtained from the structure noise maps. Double precision, in units of MJy/sr.
MJy/sr
double
name
The object name is an identifier consisting of two parts, acronym and sequence, and is formatted as ’HPPSCxxxA_Jhhmmss.s±ddmmss’. ’HPPSC’ stands for Herschel PACS Point Source Catalogue, xxx is the central wavelength of the band in which the source was observed, identifying the wavelength in microns, and the letter A indicates the first version of the catalogue. The second part has the format ’Jhhmmss.s+ddmmss’ derived from the source coordinates with ’J’ indicating a J2000 reference system, ’hhmmss.s’ is the Right Ascension in hours, minutes and seconds accuracy of one digits after the decimal, and ’+ddmmss’ is the Declination in signed degrees, minutes and seconds to an accuracy of one digit after the decimal.
meta.id;meta.main
char
primary
ra
Right Ascension coordinate in a J2000.0 reference frame. This is the peak position of the SUSSEXtractor detection. The coordinates are degrees written in double precision format.
deg
pos.eq.ra;meta.main
double
primary
dec
Declination coordinate in a J2000.0 reference frame. This is the peak position of the SUSSEXtractor detection. The coordinates are degrees written in double precision format.
deg
pos.eq.dec;meta.main
double
primary
flux
This is the flux as provided by the AnnularSkyAperturePhotometry task. For objects that were identified several times across different maps, this flux corresponds to the extraction with the best average S/N, where the Ns based S/N (S/Ns)and the background RMS based S/N (S/Nr) values are taken into account. For the blue and green bands the aperture radius was 6??, for the red band 12?? (see Section 3.3 for more details). For all cases the raw flux density values were corrected for the aperture size, based on Lutz (2015). Colour corrections were not applied. The units are mJy, written as double precision.
mJy
double
primary
rms
RMS noise as measured in the blank sky apertures placed around the source. Double precision.
mJy
double
primary
fwhmxfit
FWHM in x direction. This column contains the FWHM values measured by the 2D Gaussian model in X and Y directions, fitted by the sourceFitter() task. If the elongated Gaussian fit was possible then both FWHMx and FWHMy are listed. If only a circular Gaussian could be fitted then FWHMy is equal to -99.9. It is written in double precision format, in units of second of arc.
arcseconds
double
primary
fwhmyfit
FWHM in y direction. This column contains the FWHM values measured by the 2D Gaussian model in X and Y directions, fitted by the sourceFitter() task. If the elongated Gaussian fit was possible then both FWHMx and FWHMy are listed. If only a circular Gaussian could be fitted then FWHMy is equal to -99.9. It is written in double precision format, in units of second of arc.
arcseconds
double
primary
snr
Estimated S/N based on a statistical approach, using the S/Ns calibration surfaces. It is calculated as a function of the source flux and the Ns value. The data type is double precision.
double
primary
stn
Calculated as the ratio of the source flux and the RMS. Data type is double precision.
double
primary
elong_flag
If an elliptical Gaussian model was fitted in the source, this column contains the ratio of the FWHMy and FWHMx. A value of 0 means that the source is circular, 0.5 means that FWHMy = 0.5 × FWHMx. If FWHMy = -99.9 (circular detection), FLAG_ELONG = 0. FLAG_ELONG is also set to 0 if the source eccentricity (FWHMx - FWHMy)/FWHMx) defined in a similar way with the FWHM values of the PACS PSF reported in Table 1, is smaller than the PSF eccentricity, Double precision format.
double
primary
edge_flag
The position of a source with respect to the edges of the image affects the quality of the photometry, as the extraction procedure needs a large enough area to compute properly both the flux density and the background to be subtracted. Also, due to the scan speed inhomogeneities during the turnarounds, the map edges may have different noise properties than the rest of the image.
boolean
primary
blend_flag
Objects with distance within the PSF FWHM have the same value (>0) of FLAG_BLEND and they can be considered as blended sources. FLAG_BLEND = 0 means that the object is not blended with other objects. The PACS PSFs depend on the observing mode. The absolute pointing error for SPG13 (1.2??) is adopted as uncertainty.
double
primary
warmat
Flag indicating that the observation was affected by "warm" attitude. The term refers to spacecraft attitudes in which the star-tracker support structure is subject to thermal distortions as was not completely shaded from sunlight. This has an impact on the pointing accuracy. Data type is Boolean.
boolean
primary
ssomap_flag
Maps of solar system objects have typically been observed in tracking mode, but were reprocessed in the ’rest’ sky frame for the HPPSC, and may be contaminated by the moving targets. The affected OBSIDs are marked with an ’ssomap’ flag.
boolean
primary
obsid
The term is the observation identifier for the Herschel observations . It is a 10 digit integer, starting always with 1342. The column lists the first OBSID from the list that built the L2.5/L3 map. It corresponds to the meta keyword obsid001.
char
primary
catalogues.mv_v_hsa_cat_hppsc_160_fdw
band
This is one of the strings "blue","green","red" identifying the PACS detector array names for the filter bands centred at 70, 100, 160 microns, respectively. The wavelength is also specified in the name of the object.
microns
char
decerr
Positional uncertainties of each object as provided by SUSSEXtractor. Units are degrees, the data type is double precision.
deg
double
fratio
The ratio of the flux density values measured in the 6th and the 1st aperture, corresponding to 4?? and 9?? in the blue and green bands, and 9?? and 14?? in the red band.
double
raerr
Positional uncertainties of each object as provided by SUSSEXtractor. Units are degrees, the data type is double precision.
deg
double
snrnoise
It is calculated from the source flux and the estimated S/Ns, by dividing the flux by the S/Ns. This noise includes both the sky confusion and the instrument noise.
double
strn
Structure noise value obtained from the structure noise maps. Double precision, in units of MJy/sr.
MJy/sr
double
name
The object name is an identifier consisting of two parts, acronym and sequence, and is formatted as ’HPPSCxxxA_Jhhmmss.s±ddmmss’. ’HPPSC’ stands for Herschel PACS Point Source Catalogue, xxx is the central wavelength of the band in which the source was observed, identifying the wavelength in microns, and the letter A indicates the first version of the catalogue. The second part has the format ’Jhhmmss.s+ddmmss’ derived from the source coordinates with ’J’ indicating a J2000 reference system, ’hhmmss.s’ is the Right Ascension in hours, minutes and seconds accuracy of one digits after the decimal, and ’+ddmmss’ is the Declination in signed degrees, minutes and seconds to an accuracy of one digit after the decimal.
meta.id;meta.main
char
primary
ra
Right Ascension coordinate in a J2000.0 reference frame. This is the peak position of the SUSSEXtractor detection. The coordinates are degrees written in double precision format.
deg
pos.eq.ra;meta.main
double
primary
dec
Declination coordinate in a J2000.0 reference frame. This is the peak position of the SUSSEXtractor detection. The coordinates are degrees written in double precision format.
deg
pos.eq.dec;meta.main
double
primary
flux
This is the flux as provided by the AnnularSkyAperturePhotometry task. For objects that were identified several times across different maps, this flux corresponds to the extraction with the best average S/N, where the Ns based S/N (S/Ns)and the background RMS based S/N (S/Nr) values are taken into account. For the blue and green bands the aperture radius was 6??, for the red band 12?? (see Section 3.3 for more details). For all cases the raw flux density values were corrected for the aperture size, based on Lutz (2015). Colour corrections were not applied. The units are mJy, written as double precision.
mJy
double
primary
rms
RMS noise as measured in the blank sky apertures placed around the source. Double precision.
mJy
double
primary
fwhmxfit
FWHM in x direction. This column contains the FWHM values measured by the 2D Gaussian model in X and Y directions, fitted by the sourceFitter() task. If the elongated Gaussian fit was possible then both FWHMx and FWHMy are listed. If only a circular Gaussian could be fitted then FWHMy is equal to -99.9. It is written in double precision format, in units of second of arc.
arcseconds
double
primary
fwhmyfit
FWHM in y direction. This column contains the FWHM values measured by the 2D Gaussian model in X and Y directions, fitted by the sourceFitter() task. If the elongated Gaussian fit was possible then both FWHMx and FWHMy are listed. If only a circular Gaussian could be fitted then FWHMy is equal to -99.9. It is written in double precision format, in units of second of arc.
arcseconds
double
primary
snr
Estimated S/N based on a statistical approach, using the S/Ns calibration surfaces. It is calculated as a function of the source flux and the Ns value. The data type is double precision.
double
primary
stn
Calculated as the ratio of the source flux and the RMS. Data type is double precision.
double
primary
elong_flag
If an elliptical Gaussian model was fitted in the source, this column contains the ratio of the FWHMy and FWHMx. A value of 0 means that the source is circular, 0.5 means that FWHMy = 0.5 × FWHMx. If FWHMy = -99.9 (circular detection), FLAG_ELONG = 0. FLAG_ELONG is also set to 0 if the source eccentricity (FWHMx - FWHMy)/FWHMx) defined in a similar way with the FWHM values of the PACS PSF reported in Table 1, is smaller than the PSF eccentricity, Double precision format.
double
primary
edge_flag
The position of a source with respect to the edges of the image affects the quality of the photometry, as the extraction procedure needs a large enough area to compute properly both the flux density and the background to be subtracted. Also, due to the scan speed inhomogeneities during the turnarounds, the map edges may have different noise properties than the rest of the image.
boolean
primary
blend_flag
Objects with distance within the PSF FWHM have the same value (>0) of FLAG_BLEND and they can be considered as blended sources. FLAG_BLEND = 0 means that the object is not blended with other objects. The PACS PSFs depend on the observing mode. The absolute pointing error for SPG13 (1.2??) is adopted as uncertainty.
double
primary
warmat
Flag indicating that the observation was affected by "warm" attitude. The term refers to spacecraft attitudes in which the star-tracker support structure is subject to thermal distortions as was not completely shaded from sunlight. This has an impact on the pointing accuracy. Data type is Boolean.
boolean
primary
ssomap_flag
Maps of solar system objects have typically been observed in tracking mode, but were reprocessed in the ’rest’ sky frame for the HPPSC, and may be contaminated by the moving targets. The affected OBSIDs are marked with an ’ssomap’ flag.
boolean
primary
obsid
The term is the observation identifier for the Herschel observations . It is a 10 digit integer, starting always with 1342. The column lists the first OBSID from the list that built the L2.5/L3 map. It corresponds to the meta keyword obsid001.
char
primary
catalogues.mv_v_hsa_cat_spsc_250_fdw
astrom_flag
Astrometry flag indicating that one or more of the contributing source detections came from a map with a positional offset greater than 5” derived from stacking at WISE 24 ?m catalog positions. A total of 140573 records was flagged in this way.
char
conf_err
This column indicates the local confusion uncertainty in mJy. It is the average of the individual values of all contributing sources, weighted with the respective TML uncertainties.
mJy
double
dec_err
Positional uncertainty in arcsec of each catalog object. It is derived as the larger of either quadratic mean of all the individual TML uncertainties of all contributing source detections or the standard deviation of all source positions, divided by the square root of the number of maps the source is detected in.
arcseconds
double
det
This is one of the strings “PSW”, “PMW”, “PLW” identifying the SPIRE detector array names for the filter bands centered at 250, 350, 500 microns respectively. This column is for convenience for those more familiar with the instrument specific naming. Otherwise the wavelength is indicated in the object identifier.
char
dupl_flag
This flag is False by default and set to True if more than one source from the same map were identified as part of this object by the object consolidation algorithm. This is a rare occurrence and mainly due to limitations of the algorithm used. The flag was set 1624 times (960,497,167 for the filter bands respectively).
char
fluxsus
This column shows the average of the Sussextractor derived fluxes of all contributing sources, weighted with the respective Sussextractor generated uncertainties.
mJy
double
fluxsus_err
This column contains the propagated weighted error produced by Sussextractor for all contributing source detections.
mJy
double
fluxtml_err
This column contains the propagated weighted error produced by the TML for all contributing source detections.
mJy
double
fwhm1
This column contains the average FWHM of the major axes of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections, weighted by their respective uncertainties.
arcseconds
double
fwhm1_err
This column contains the respective uncertainties of the weighted averages of the major and minor axes of the fitted elliptical Gaussian beam profile in arcsec.
arcseconds
double
fwhm2
This column contains the average FWHM of the minor axes of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections, weighted by their respective uncertainties.
arcseconds
double
fwhm2_err
This column contains the respective uncertainties of the weighted averages of the major and minor axes of the fitted elliptical Gaussian beam profile in arcsec.
arcseconds
double
insterr_flag
This flag indicates that the TML returned no count for the number of readouts in the central aperture. To still be able to derive an instrument noise component, a typical number was used, based on the instrument configuration and multiplied with the number of repeats of the observation.
char
ndet
This column contains the actual number of detections in separate maps of this object at this position and filter band. Combinations of maps into a Level 2.5 map are counted as one. There are rare cases where two close, but separate detections in the same map become part of the same object because the grouping algorithm was not able to distinguish them. In this case the source duplication flag is set.
int
nmap
The number of times a source should have been detected at the list position and in the same band pass, based on the coverage maps. This value is derived by testing a 3x3 pixel square centered on the source in each coverage map. If the coverage anywhere within this square is greater than zero, the NMAP value for this object is incremented by one.
int
pos_flag
This flag indicates a potential problem with the position of this source if set to True. It is set if the uncertainties associated with the position are larger than the search radius used by the consolidation algorithm. It is also set if the maximum distance between the positions of all contributing detections is larger than the search radius used by the consolidation algorithm. The search radius is chosen as half of the FWHM of the beam profile for the respective source increased by 6” as allowance for the 3 sigma pointing uncertainty of Herschel
char
q3ctile
As the exclusion criterion for regions with highly structured background emission is determined on the basis of the median STRN within a Q3C tile at the 22 bit level, we add the respective Q3C tile identifier to each object. It is a 19 digit number that is best interpreted using the Postgres implementation of Q3C.
double
ra_err
Positional uncertainty in arcsec of each catalog object. It is derived as the larger of either quadratic mean of all the individual TML uncertainties of all contributing source detections or the standard deviation of all source positions, divided by the square root of the number of maps the source is detected in.
arcseconds
double
rot
This column contains a robust average rotation angle of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections. Robust meaning that all angles with uncertainties that are larger than a factor 1.5 of the median of all uncertainties of the contributing detections are removed before averaging. The rotation angle on the sky is measured from West counter-clockwise in degrees. Possible values start from 0 and are smaller than 180 deg. The average of the angles is calculated in Cartesian space to avoid problems when crossing the 180 deg threshold. Since a position angle of 180 deg is equal to 0 deg, we multiplied the position angles by 2 before averaging and divided by 2 after the back-transformation. A constant of 180 deg was added when the angle was smaller than 0 to stay within the allowed range.
deg
double
rot_err
This column contains the propagated error of the rotation angle for all contributing source detections.
deg
double
name
The object identifier consists of two parts, acronym and sequence, and is formatted as “HSPSCwwwA_Jhhmm.mm+ddmm.m” with the exception of the planets Uranus and Neptune, which are following the format “HSPSCwwwA_ppp_000”. “HSPSC” stands for Herschel SPIRE Point Source Catalog, “www” is one of [250,350,500], identifying the wavelength in microns, and the letter A indicates the first public version of the catalog. The sequence has the format “Jhhmm.mm+ddmm.m”, which is derived from the object coordinates with J indicating a J2000 reference system, “hhmm.mm” indicating the Right Ascension in hours and minutes to an accuracy of two digits after the decimal, and “+ddmm.m” indicating Declination in signed degrees and minutes to an accuracy of one digit after the decimal. In the case of the planets the sequence is formatted as “ppp_000”, where “ppp” stands for one of the strings “URA” or “NEP” indicating Uranus or Neptune respectively, followed by a running number “000” indicating the observation. The spatial resolution of the coordinate based serial number is well matched to the size of SPIRE’s beam profiles and will keep changes in object names to a minimum if another version of the catalog is generated.
meta.id;meta.main
char
primary
ra
Right Ascension coordinate in a J2000.0 reference frame, calculated as the average of the Right Ascensions of all the contributing source detections in different maps. The positions used result from the refined Timeline Fitter positions and their uncertainties. The average is calculated in Cartesian space and transformed back to spherical coordinates to avoid problems near the celestial poles.
deg
pos.eq.ra;meta.main
double
primary
dec
Declination coordinate in a J2000.0 reference frame, calculated as the average of the Right Ascensions of all the contributing source detections in different maps. The positions used result from the refined Timeline Fitter positions and their uncertainties. The average is calculated in Cartesian space and transformed back to spherical coordinates to avoid problems near the celestial poles.
deg
pos.eq.dec;meta.main
double
primary
snr
This value has been added for convenience and expresses the signal to noise ratio associated with a given object as the ratio between the Timeline Fitter flux (FLUX) and the total flux error (FLUX_ERR).
double
primary
flux
This column shows the average of the TML derived fluxes of all contributing sources, weighted with the respective TML generated uncertainties. This procedure of fitting a fixed width circular Gaussian beam profile model has proven to be superior to a number of other common methods used with SPIRE data in terms of reproducibility and photometric accuracy, down to fluxes of 30 mJy (Pearson et al. 2014).
mJy
double
primary
flux_err
This column indicates the local confusion uncertainty in mJy. It is the average of the individual values of all contributing sources, weighted with the respective TML uncertainties.
mJy
double
primary
fluxdao
This column shows the average of the Daophot derived fluxes of all contributing sources, weighted with the respective Daophot generated uncertainties.
mJy
double
primary
fluxdao_err
This column contains the propagated weighted error produced by Daophot for all contributing source detections.
mJy
double
primary
fluxtm2
This column shows the average of the TM2 derived fluxes of all contributing sources, weighted with the respective TM2 generated uncertainties. This procedure fits an elliptical Gaussian beam profile model where the major and minor axes have been left as free fit parameters. The configuration also allows for a tilted background plane.
mJy
double
primary
fluxtm2_err
This column contains the propagated weighted error produced by TML2 for all contributing source detections.
mJy
double
primary
pntsrc_flag
The flag is set for all objects, where both the major and minor FWHM parameters are still compatible with values that are observed from point sources at a given flux level. As such it is an indicator but not conclusive, in particular not for small fluxes.
char
primary
extsrc_flag
This flag is set if any of the major or minor FWHM is larger than the upper flux dependent threshold for point sources.
char
primary
lowfwhm_flag
This flag is set if any of the major or minor FWHM is smaller than the lower flux dependent threshold for point sources.
char
primary
largegal_flag
This flag is set when the catalog position is within one of the ellipses given in the 2MASS Large Galaxy Atlas (LGA) (Jarrett et al 2003) for galaxies with major axis > 1arcmin. The values are described as 'K_s (LGA/2MASS "total")' and represent the standard 2MASS aperture. If the flag is set there is a high probability that the source is part of the respective large galaxy rather than a background object.
char
primary
mapedge_flag
The map edge flag is set when at least one of the contributing sources shows 10 or more percent of map pixels without a flux value (NaN) within the outer radius of the background annulus used by the Timeline Fitter (74”, 103”, 147”) for 250, 350, and 500 microns respectively. This condition flags catalog objects where its detection or the flux estimate may have been affected by at least one contributor being close to a map edge. 24313 objects are the edge flag set.
char
primary
ssocont_flag
This flag is set as a warning if any of the known contributors to the catalog object is within a rectangle defined by the tracklet of a known asteroid at the time of the observation of the respective map, and the beam FWHM at the wavelength of the map. The estimated flux using a simple asteroid standard model needs to be at least at the one sigma confusion limit of Nguyen et al. (2010) of 5.8, 6.3, 6.8 mJy for 250, 350, and 500 microns respectively. 810 objects have this flag set.
char
primary
catalogues.mv_v_hsa_cat_spsc_350_fdw
astrom_flag
Astrometry flag indicating that one or more of the contributing source detections came from a map with a positional offset greater than 5” derived from stacking at WISE 24 ?m catalog positions. A total of 140573 records was flagged in this way.
char
conf_err
This column indicates the local confusion uncertainty in mJy. It is the average of the individual values of all contributing sources, weighted with the respective TML uncertainties.
mJy
double
dec_err
Positional uncertainty in arcsec of each catalog object. It is derived as the larger of either quadratic mean of all the individual TML uncertainties of all contributing source detections or the standard deviation of all source positions, divided by the square root of the number of maps the source is detected in.
arcseconds
double
det
This is one of the strings “PSW”, “PMW”, “PLW” identifying the SPIRE detector array names for the filter bands centered at 250, 350, 500 microns respectively. This column is for convenience for those more familiar with the instrument specific naming. Otherwise the wavelength is indicated in the object identifier.
char
dupl_flag
This flag is False by default and set to True if more than one source from the same map were identified as part of this object by the object consolidation algorithm. This is a rare occurrence and mainly due to limitations of the algorithm used. The flag was set 1624 times (960,497,167 for the filter bands respectively).
char
fluxsus
This column shows the average of the Sussextractor derived fluxes of all contributing sources, weighted with the respective Sussextractor generated uncertainties.
mJy
double
fluxsus_err
This column contains the propagated weighted error produced by Sussextractor for all contributing source detections.
mJy
double
fluxtml_err
This column contains the propagated weighted error produced by the TML for all contributing source detections.
mJy
double
fwhm1
This column contains the average FWHM of the major axes of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections, weighted by their respective uncertainties.
arcseconds
double
fwhm1_err
This column contains the respective uncertainties of the weighted averages of the major and minor axes of the fitted elliptical Gaussian beam profile in arcsec.
arcseconds
double
fwhm2
This column contains the average FWHM of the minor axes of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections, weighted by their respective uncertainties.
arcseconds
double
fwhm2_err
This column contains the respective uncertainties of the weighted averages of the major and minor axes of the fitted elliptical Gaussian beam profile in arcsec.
arcseconds
double
insterr_flag
This flag indicates that the TML returned no count for the number of readouts in the central aperture. To still be able to derive an instrument noise component, a typical number was used, based on the instrument configuration and multiplied with the number of repeats of the observation.
char
ndet
This column contains the actual number of detections in separate maps of this object at this position and filter band. Combinations of maps into a Level 2.5 map are counted as one. There are rare cases where two close, but separate detections in the same map become part of the same object because the grouping algorithm was not able to distinguish them. In this case the source duplication flag is set.
int
nmap
The number of times a source should have been detected at the list position and in the same band pass, based on the coverage maps. This value is derived by testing a 3x3 pixel square centered on the source in each coverage map. If the coverage anywhere within this square is greater than zero, the NMAP value for this object is incremented by one.
int
pos_flag
This flag indicates a potential problem with the position of this source if set to True. It is set if the uncertainties associated with the position are larger than the search radius used by the consolidation algorithm. It is also set if the maximum distance between the positions of all contributing detections is larger than the search radius used by the consolidation algorithm. The search radius is chosen as half of the FWHM of the beam profile for the respective source increased by 6” as allowance for the 3 sigma pointing uncertainty of Herschel
char
q3ctile
As the exclusion criterion for regions with highly structured background emission is determined on the basis of the median STRN within a Q3C tile at the 22 bit level, we add the respective Q3C tile identifier to each object. It is a 19 digit number that is best interpreted using the Postgres implementation of Q3C.
double
ra_err
Positional uncertainty in arcsec of each catalog object. It is derived as the larger of either quadratic mean of all the individual TML uncertainties of all contributing source detections or the standard deviation of all source positions, divided by the square root of the number of maps the source is detected in.
arcseconds
double
rot
This column contains a robust average rotation angle of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections. Robust meaning that all angles with uncertainties that are larger than a factor 1.5 of the median of all uncertainties of the contributing detections are removed before averaging. The rotation angle on the sky is measured from West counter-clockwise in degrees. Possible values start from 0 and are smaller than 180 deg. The average of the angles is calculated in Cartesian space to avoid problems when crossing the 180 deg threshold. Since a position angle of 180 deg is equal to 0 deg, we multiplied the position angles by 2 before averaging and divided by 2 after the back-transformation. A constant of 180 deg was added when the angle was smaller than 0 to stay within the allowed range.
deg
double
rot_err
This column contains the propagated error of the rotation angle for all contributing source detections.
deg
double
name
The object identifier consists of two parts, acronym and sequence, and is formatted as “HSPSCwwwA_Jhhmm.mm+ddmm.m” with the exception of the planets Uranus and Neptune, which are following the format “HSPSCwwwA_ppp_000”. “HSPSC” stands for Herschel SPIRE Point Source Catalog, “www” is one of [250,350,500], identifying the wavelength in microns, and the letter A indicates the first public version of the catalog. The sequence has the format “Jhhmm.mm+ddmm.m”, which is derived from the object coordinates with J indicating a J2000 reference system, “hhmm.mm” indicating the Right Ascension in hours and minutes to an accuracy of two digits after the decimal, and “+ddmm.m” indicating Declination in signed degrees and minutes to an accuracy of one digit after the decimal. In the case of the planets the sequence is formatted as “ppp_000”, where “ppp” stands for one of the strings “URA” or “NEP” indicating Uranus or Neptune respectively, followed by a running number “000” indicating the observation. The spatial resolution of the coordinate based serial number is well matched to the size of SPIRE’s beam profiles and will keep changes in object names to a minimum if another version of the catalog is generated.
meta.id;meta.main
char
primary
ra
Right Ascension coordinate in a J2000.0 reference frame, calculated as the average of the Right Ascensions of all the contributing source detections in different maps. The positions used result from the refined Timeline Fitter positions and their uncertainties. The average is calculated in Cartesian space and transformed back to spherical coordinates to avoid problems near the celestial poles.
deg
pos.eq.ra;meta.main
double
primary
dec
Declination coordinate in a J2000.0 reference frame, calculated as the average of the Right Ascensions of all the contributing source detections in different maps. The positions used result from the refined Timeline Fitter positions and their uncertainties. The average is calculated in Cartesian space and transformed back to spherical coordinates to avoid problems near the celestial poles.
deg
pos.eq.dec;meta.main
double
primary
snr
This value has been added for convenience and expresses the signal to noise ratio associated with a given object as the ratio between the Timeline Fitter flux (FLUX) and the total flux error (FLUX_ERR).
double
primary
flux
This column shows the average of the TML derived fluxes of all contributing sources, weighted with the respective TML generated uncertainties. This procedure of fitting a fixed width circular Gaussian beam profile model has proven to be superior to a number of other common methods used with SPIRE data in terms of reproducibility and photometric accuracy, down to fluxes of 30 mJy (Pearson et al. 2014).
mJy
double
primary
flux_err
This column indicates the local confusion uncertainty in mJy. It is the average of the individual values of all contributing sources, weighted with the respective TML uncertainties.
mJy
double
primary
fluxdao
This column shows the average of the Daophot derived fluxes of all contributing sources, weighted with the respective Daophot generated uncertainties.
mJy
double
primary
fluxdao_err
This column contains the propagated weighted error produced by Daophot for all contributing source detections.
mJy
double
primary
fluxtm2
This column shows the average of the TM2 derived fluxes of all contributing sources, weighted with the respective TM2 generated uncertainties. This procedure fits an elliptical Gaussian beam profile model where the major and minor axes have been left as free fit parameters. The configuration also allows for a tilted background plane.
mJy
double
primary
fluxtm2_err
This column contains the propagated weighted error produced by TML2 for all contributing source detections.
mJy
double
primary
pntsrc_flag
The flag is set for all objects, where both the major and minor FWHM parameters are still compatible with values that are observed from point sources at a given flux level. As such it is an indicator but not conclusive, in particular not for small fluxes.
char
primary
extsrc_flag
This flag is set if any of the major or minor FWHM is larger than the upper flux dependent threshold for point sources.
char
primary
lowfwhm_flag
This flag is set if any of the major or minor FWHM is smaller than the lower flux dependent threshold for point sources.
char
primary
largegal_flag
This flag is set when the catalog position is within one of the ellipses given in the 2MASS Large Galaxy Atlas (LGA) (Jarrett et al 2003) for galaxies with major axis > 1arcmin. The values are described as 'K_s (LGA/2MASS "total")' and represent the standard 2MASS aperture. If the flag is set there is a high probability that the source is part of the respective large galaxy rather than a background object.
char
primary
mapedge_flag
The map edge flag is set when at least one of the contributing sources shows 10 or more percent of map pixels without a flux value (NaN) within the outer radius of the background annulus used by the Timeline Fitter (74”, 103”, 147”) for 250, 350, and 500 microns respectively. This condition flags catalog objects where its detection or the flux estimate may have been affected by at least one contributor being close to a map edge. 24313 objects are the edge flag set.
char
primary
ssocont_flag
This flag is set as a warning if any of the known contributors to the catalog object is within a rectangle defined by the tracklet of a known asteroid at the time of the observation of the respective map, and the beam FWHM at the wavelength of the map. The estimated flux using a simple asteroid standard model needs to be at least at the one sigma confusion limit of Nguyen et al. (2010) of 5.8, 6.3, 6.8 mJy for 250, 350, and 500 microns respectively. 810 objects have this flag set.
char
primary
catalogues.mv_v_hsa_cat_spsc_500_fdw
astrom_flag
Astrometry flag indicating that one or more of the contributing source detections came from a map with a positional offset greater than 5” derived from stacking at WISE 24 ?m catalog positions. A total of 140573 records was flagged in this way.
char
conf_err
This column indicates the local confusion uncertainty in mJy. It is the average of the individual values of all contributing sources, weighted with the respective TML uncertainties.
mJy
double
dec_err
Positional uncertainty in arcsec of each catalog object. It is derived as the larger of either quadratic mean of all the individual TML uncertainties of all contributing source detections or the standard deviation of all source positions, divided by the square root of the number of maps the source is detected in.
arcseconds
double
det
This is one of the strings “PSW”, “PMW”, “PLW” identifying the SPIRE detector array names for the filter bands centered at 250, 350, 500 microns respectively. This column is for convenience for those more familiar with the instrument specific naming. Otherwise the wavelength is indicated in the object identifier.
char
dupl_flag
This flag is False by default and set to True if more than one source from the same map were identified as part of this object by the object consolidation algorithm. This is a rare occurrence and mainly due to limitations of the algorithm used. The flag was set 1624 times (960,497,167 for the filter bands respectively).
char
fluxsus
This column shows the average of the Sussextractor derived fluxes of all contributing sources, weighted with the respective Sussextractor generated uncertainties.
mJy
double
fluxsus_err
This column contains the propagated weighted error produced by Sussextractor for all contributing source detections.
mJy
double
fluxtml_err
This column contains the propagated weighted error produced by the TML for all contributing source detections.
mJy
double
fwhm1
This column contains the average FWHM of the major axes of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections, weighted by their respective uncertainties.
arcseconds
double
fwhm1_err
This column contains the respective uncertainties of the weighted averages of the major and minor axes of the fitted elliptical Gaussian beam profile in arcsec.
arcseconds
double
fwhm2
This column contains the average FWHM of the minor axes of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections, weighted by their respective uncertainties.
arcseconds
double
fwhm2_err
This column contains the respective uncertainties of the weighted averages of the major and minor axes of the fitted elliptical Gaussian beam profile in arcsec.
arcseconds
double
insterr_flag
This flag indicates that the TML returned no count for the number of readouts in the central aperture. To still be able to derive an instrument noise component, a typical number was used, based on the instrument configuration and multiplied with the number of repeats of the observation.
char
ndet
This column contains the actual number of detections in separate maps of this object at this position and filter band. Combinations of maps into a Level 2.5 map are counted as one. There are rare cases where two close, but separate detections in the same map become part of the same object because the grouping algorithm was not able to distinguish them. In this case the source duplication flag is set.
int
nmap
The number of times a source should have been detected at the list position and in the same band pass, based on the coverage maps. This value is derived by testing a 3x3 pixel square centered on the source in each coverage map. If the coverage anywhere within this square is greater than zero, the NMAP value for this object is incremented by one.
int
pos_flag
This flag indicates a potential problem with the position of this source if set to True. It is set if the uncertainties associated with the position are larger than the search radius used by the consolidation algorithm. It is also set if the maximum distance between the positions of all contributing detections is larger than the search radius used by the consolidation algorithm. The search radius is chosen as half of the FWHM of the beam profile for the respective source increased by 6” as allowance for the 3 sigma pointing uncertainty of Herschel
char
q3ctile
As the exclusion criterion for regions with highly structured background emission is determined on the basis of the median STRN within a Q3C tile at the 22 bit level, we add the respective Q3C tile identifier to each object. It is a 19 digit number that is best interpreted using the Postgres implementation of Q3C.
double
ra_err
Positional uncertainty in arcsec of each catalog object. It is derived as the larger of either quadratic mean of all the individual TML uncertainties of all contributing source detections or the standard deviation of all source positions, divided by the square root of the number of maps the source is detected in.
arcseconds
double
rot
This column contains a robust average rotation angle of the elliptical Gaussian beam profile models fitted during the TM2 run to all the contributing detections. Robust meaning that all angles with uncertainties that are larger than a factor 1.5 of the median of all uncertainties of the contributing detections are removed before averaging. The rotation angle on the sky is measured from West counter-clockwise in degrees. Possible values start from 0 and are smaller than 180 deg. The average of the angles is calculated in Cartesian space to avoid problems when crossing the 180 deg threshold. Since a position angle of 180 deg is equal to 0 deg, we multiplied the position angles by 2 before averaging and divided by 2 after the back-transformation. A constant of 180 deg was added when the angle was smaller than 0 to stay within the allowed range.
deg
double
rot_err
This column contains the propagated error of the rotation angle for all contributing source detections.
deg
double
name
The object identifier consists of two parts, acronym and sequence, and is formatted as “HSPSCwwwA_Jhhmm.mm+ddmm.m” with the exception of the planets Uranus and Neptune, which are following the format “HSPSCwwwA_ppp_000”. “HSPSC” stands for Herschel SPIRE Point Source Catalog, “www” is one of [250,350,500], identifying the wavelength in microns, and the letter A indicates the first public version of the catalog. The sequence has the format “Jhhmm.mm+ddmm.m”, which is derived from the object coordinates with J indicating a J2000 reference system, “hhmm.mm” indicating the Right Ascension in hours and minutes to an accuracy of two digits after the decimal, and “+ddmm.m” indicating Declination in signed degrees and minutes to an accuracy of one digit after the decimal. In the case of the planets the sequence is formatted as “ppp_000”, where “ppp” stands for one of the strings “URA” or “NEP” indicating Uranus or Neptune respectively, followed by a running number “000” indicating the observation. The spatial resolution of the coordinate based serial number is well matched to the size of SPIRE’s beam profiles and will keep changes in object names to a minimum if another version of the catalog is generated.
meta.id;meta.main
char
primary
ra
Right Ascension coordinate in a J2000.0 reference frame, calculated as the average of the Right Ascensions of all the contributing source detections in different maps. The positions used result from the refined Timeline Fitter positions and their uncertainties. The average is calculated in Cartesian space and transformed back to spherical coordinates to avoid problems near the celestial poles.
deg
pos.eq.ra;meta.main
double
primary
dec
Declination coordinate in a J2000.0 reference frame, calculated as the average of the Right Ascensions of all the contributing source detections in different maps. The positions used result from the refined Timeline Fitter positions and their uncertainties. The average is calculated in Cartesian space and transformed back to spherical coordinates to avoid problems near the celestial poles.
deg
pos.eq.dec;meta.main
double
primary
snr
This value has been added for convenience and expresses the signal to noise ratio associated with a given object as the ratio between the Timeline Fitter flux (FLUX) and the total flux error (FLUX_ERR).
double
primary
flux
This column shows the average of the TML derived fluxes of all contributing sources, weighted with the respective TML generated uncertainties. This procedure of fitting a fixed width circular Gaussian beam profile model has proven to be superior to a number of other common methods used with SPIRE data in terms of reproducibility and photometric accuracy, down to fluxes of 30 mJy (Pearson et al. 2014).
mJy
double
primary
flux_err
This column indicates the local confusion uncertainty in mJy. It is the average of the individual values of all contributing sources, weighted with the respective TML uncertainties.
mJy
double
primary
fluxdao
This column shows the average of the Daophot derived fluxes of all contributing sources, weighted with the respective Daophot generated uncertainties.
mJy
double
primary
fluxdao_err
This column contains the propagated weighted error produced by Daophot for all contributing source detections.
mJy
double
primary
fluxtm2
This column shows the average of the TM2 derived fluxes of all contributing sources, weighted with the respective TM2 generated uncertainties. This procedure fits an elliptical Gaussian beam profile model where the major and minor axes have been left as free fit parameters. The configuration also allows for a tilted background plane.
mJy
double
primary
fluxtm2_err
This column contains the propagated weighted error produced by TML2 for all contributing source detections.
mJy
double
primary
pntsrc_flag
The flag is set for all objects, where both the major and minor FWHM parameters are still compatible with values that are observed from point sources at a given flux level. As such it is an indicator but not conclusive, in particular not for small fluxes.
char
primary
extsrc_flag
This flag is set if any of the major or minor FWHM is larger than the upper flux dependent threshold for point sources.
char
primary
lowfwhm_flag
This flag is set if any of the major or minor FWHM is smaller than the lower flux dependent threshold for point sources.
char
primary
largegal_flag
This flag is set when the catalog position is within one of the ellipses given in the 2MASS Large Galaxy Atlas (LGA) (Jarrett et al 2003) for galaxies with major axis > 1arcmin. The values are described as 'K_s (LGA/2MASS "total")' and represent the standard 2MASS aperture. If the flag is set there is a high probability that the source is part of the respective large galaxy rather than a background object.
char
primary
mapedge_flag
The map edge flag is set when at least one of the contributing sources shows 10 or more percent of map pixels without a flux value (NaN) within the outer radius of the background annulus used by the Timeline Fitter (74”, 103”, 147”) for 250, 350, and 500 microns respectively. This condition flags catalog objects where its detection or the flux estimate may have been affected by at least one contributor being close to a map edge. 24313 objects are the edge flag set.
char
primary
ssocont_flag
This flag is set as a warning if any of the known contributors to the catalog object is within a rectangle defined by the tracklet of a known asteroid at the time of the observation of the respective map, and the beam FWHM at the wavelength of the map. The estimated flux using a simple asteroid standard model needs to be at least at the one sigma confusion limit of Nguyen et al. (2010) of 5.8, 6.3, 6.8 mJy for 250, 350, and 500 microns respectively. 810 objects have this flag set.
char
primary
catalogues.mv_v_icecubepsc_fdw
"time"
double
"__row"
system index column
char
event_number
Sequential Number Assigned by the HEASARC to Each Event in the Catalog
meta.id
int
primary
ra
Right Ascension
degree
pos.eq.ra;meta.main
double
primary
dec
Declination
degree
pos.eq.dec;meta.main
double
primary
lii
Galactic Longitude
degree
pos.galactic.lon
double
bii
Galactic Latitude
degree
pos.galactic.lat
double
error_radius
Positional Uncertainty
degree
stat.error;pos
double
primary
event_time
Date/Time of the Event
time.start;obs
char
primary
azimuth
Local Azimuth Coordinate
degree
pos.az.azi
double
event_energy
Reconstructed Energy of the Observed Muon Track
GeV
phys.energy
double
primary
zenith
Local Zenith Coordinate
degree
pos.az.zd
double
config_code
IceCube Detector Configuration Code
meta.code;instr.det
char
"__x_ra_dec"
system unit vector column
double
"__y_ra_dec"
system unit vector column
double
"__z_ra_dec"
system unit vector column
double
icecubepsc_oid
meta.oid
int
npix
Healpix pixel of the center of the observation for nside 256
long
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
catalogues.mv_v_sz_catalog_fdw
pos
pgsphere spoint representation of the position (ra, dec)
radians
char
name
Source name
meta.id;meta.main
char
primary
ra
Right ascension (J2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination (J2000)
deg
pos.eq.dec;meta.main
double
primary
snr
Signal-to-noise ratio of the detection
float
primary
redshift
Redshift of cluster
float
primary
msz
Sundyaev-Zeldovitch mass proxy
10e+14 Msun
float
primary
validation
External validation status
int
primary
catalogues.mv_v_xsa_slew_source_cat_fdw
altident
An alternative name for the best match source.
char
bg_map_b6
Background value for the soft band. (0.2-2.0 keV)
counts/pixel
double
bg_map_b7
Background value for the hard band. (2.0-12.0 keV)
counts/pixel
double
bg_map_b8
Background value for the total band. (0.2-12.0 keV)
counts/pixel
double
bii
Galactic Latitude [degrees]
deg
double
bii_b6
The galactic position in [degrees] of the soft band source. (0.2-2.0 keV)
deg
double
bii_b7
The galactic position in [degrees] of the hard band source. (2.0-12.0 keV)
deg
double
bii_b8
The galactic position in [degrees] of the total band source. (0.2-12.0 keV)
deg
double
date_end
SLEW exposure end date
char
date_obs
SLEW exposure start date
char
dec_b6
The J2000 celestial position of of the soft band source. (0.2-2.0 keV)
deg
double
dec_b7
The J2000 celestial position of of the hard band source. (2.0-12.0 keV)
deg
double
dec_b8
The J2000 celestial position of of the total band source. (0.2-12.0 keV)
deg
double
det_ml_b6
The detection likelihood in the soft (0.2-2.0 keV) energy band
double
det_ml_b7
The detection likelihood in the hard (2.0-12 keV) energy band
double
det_ml_b8
The detection likelihood in the total (0.2-12 keV) energy band
double
duration
Exposure on time
pixels
int
exp_map_b6
The effective on-axis exposure time in [seconds], in the soft energy band. (0.2-2.0 keV)
seconds
double
exp_map_b7
The effective on-axis exposure time in [seconds], in the hard energy band. (2.0-12.0 keV)
seconds
double
exp_map_b8
The effective on-axis exposure time in [seconds], in the total energy band. (0.2-12.0 keV)
seconds
double
ext_b6
Spatial extension of the source in the soft energy band. (0.2-2.0 keV)
pixels
double
ext_b6_err
Statistical one sigma error on the soft band extension parameter. (0.2-2.0 keV)
pixels
double
ext_b7
Spatial extension of the source in the hard energy band. (2.0-12.0 keV)
pixels
double
ext_b7_err
Statistical one sigma error on the hard band extension parameter. (2.0-12.0 keV)
pixels
double
ext_b8
Spatial extension of the source in the total energy band. (0.2-12.0 keV)
pixels
double
ext_b8_err
Statistical one sigma error on the total band extension parameter. (0.2-12.0 keV)
pixels
double
ext_ml_b6
Likelihood of the source being extended in the soft (0.2-2 keV) energy band
double
ext_ml_b7
Likelihood of the source being extended in the hard (2-12 keV) energy band
double
ext_ml_b8
Likelihood of the source being extended in the total (0.2-12 keV) energy band.
double
filt_cnts
The number of counts found within a 1 arcminute radius about the source position after standard filtering is applied.
double
flag_comment
A comment which explains why a particular source flag has been set to true
char
hr1
The hardness ratio, defined as HR1 = (rate_b7-rate_b6)/(rate_b7+rate_b6) where rate_b7 is the hard band count rate and rate_b6 is the soft band count rate. This has been calculated for the 1936 sources which have a positive detection in both bands
double
hr1_err
Error on the hardness ratio calculated as: sqrt(rate_b7_err*rate_b7_err + rate_b6_err*rate_b6_err) /(rate_b7+rate_b6) where rate_b7_err and rate_b6_err are the errors on the hard and soft band count rates respectively
double
id_category
The source type as returned by SIMBAD, NED and the other resources used in the cross-matching process.
char
id_dist
The distance in arcminutes between the best match candidate and the SLEW survey source
arcsec
double
ident
Cross-correlations of the positions of the slew sources with astronomical databases and catalogues have been performed (see section on IDs)
char
id_resource
The astronomical database or catalogue from which the best match has been selected.
char
image_bg_rate
Peak background count rate in the image from which the source was extracted
counts/s
double
lii
Galactic Longitude [degrees]
deg
double
lii_b6
The galactic position in [degrees] of the soft band source. (0.2-2.0 keV)
deg
double
lii_b7
The galactic position in [degrees] of the hard band source. (2.0-12.0 keV)
deg
double
lii_b8
The galactic position in [degrees] of the total band source. (0.2-12.0 keV)
deg
double
mjd_start
Modified Julian Date (i.e., JD - 2400000.5) of the start of the observation.
double
mjd_stop
Modified Julian Date (i.e., JD - 2400000.5) of the end of the observation.
double
mode_id
Observing mode of the EPIC-pn camera. FF= Full frame mode eFF = extended full frame mode LW = large window mode
char
npix
Healpix pixel of the center for nside 256
long
pos
Position of the source
char
postcard_url
URL for the postcard
meta.ref.url;meta.preview
char
ra_b6
The J2000 celestial position of the soft band source. (0.2-2.0 keV)
deg
double
ra_b7
The J2000 celestial position of the hard band source. (2.0-12.0 keV)
deg
double
ra_b8
The J2000 celestial position of the total band source. (0.2-12.0 keV)
deg
double
radec_b6_err
The statistical error in [degrees], on the soft band position. (0.2-2.0 keV)
deg
double
radec_b7_err
The statistical error in [degrees], on the hard band position. (2.0-12.0 keV)
deg
double
radec_b8_err
The statistical error in [degrees], on the total band position. (0.2-12.0 keV)
deg
double
radec_err
Radial error on the position, computed as sqrt(ra_err2 + dec_err2), in arcsecs, where ra_err and dec_err are the 1 sigma uncertainties in the RA and DEC coordinates respectively.
arcsec
double
rass_dist
The distance from the best match ROSAT source and the SLEW source
arcsec
double
rassname
char
rate_b6
The soft band count rate (0.2-2.0 keV)
counts/s
double
rate_b6_err
The error on the soft band count rate (0.2-2.0 keV)
counts/s
double
rate_b7
The hard band count rate (2.0-12.0 keV)
counts/s
double
rate_b7_err
The error on the hard band count rate (2.0-12.0 keV)
counts/s
double
rate_b8
The total band count rate (0.2-12.0 keV)
counts/s
double
rate_b8_err
The error on the total band count rate (0.2-12.0 keV)
counts/s
double
scts_b6
The number of background subtracted counts, in the soft energy band (0.2-2 keV), corrected for the PSF
counts
double
scts_b6_err
Statistical 1 sigma error on the soft band source counts (0.2-2.0 keV).
counts
double
scts_b7
The number of background subtracted counts, in the hard energy band (2.0-12.0 keV)
counts
double
scts_b7_err
Statistical 1 sigma error on the hard band source counts (2.0-12.0 keV)
counts
double
scts_b8
The number of background subtracted counts, in the total energy band (0.2-12.0 keV)
counts
double
scts_b8_err
Statistical 1 sigma error on the total band source counts (0.2-12.0 keV)
counts
double
slew_observation_id
SLEW observation ID
char
slew_source_cat_fov_scircle
char
slew_source_cat_galactic_spoint
char
slew_source_cat_oid
int
srcname_b6
The source name defined in the soft band list. The format is 'xs' followed by the revolution number, the observation ID and the source position, e.g. xs0841_9084100002_12:57:07.5+01:50:42
char
srcname_b7
The source name defined in the hard band list. The format is 'xs' followed by the revolution number, the observation ID and the source position, e.g. xs0841_9084100002_12:57:07.5+01:50:42
char
srcname_b8
The source name defined in the total band list. The format is 'xs' followed by the revolution number, the observation ID and the source position, e.g. xs0841_9084100002_12:57:07.5+01:50:42
char
srcnum
This is the official name for sources detected in the XMM-Newton slew survey
int
unfilt_cnts
The number of counts found within a 1 arcminute radius about the source position with no filtering applied
double
us_extras
Name in the EXTRAS catalogue
double
us_xmmsl1
XMMSL1 name
char
val_flag
A text string which is set to 'CLEAN_SAMPLE' if this source is included in the clean subset
char
ver_false
This is a catch-all for problems not included in the other flags.
char
ver_halo
If set true, this flag indicates that a detection lies within the point spread function, or halo, of a very bright source and is probably spurious.
char
ver_hibgnd
If set true, this flag indicates that the source lies within a bright region, caused by high background, and is probably spurious.
char
ver_inext
If set true, this flag notes that a detection has been found within an extended source and is probably false. This flag is used to ensure that only one source is quoted for the large supernova remnants.
char
ver_nredg
Source near edge. Not used in XMMSL2.
char
ver_optload
A warning flag indicating that the source may suffer from optical loading
char
ver_psusp
This flag indicates that the quoted position of the source is likely to be inaccurate. In a few slews the attitude reconstruction is poor and in these cases the actual position of the source is difficult to determine and can be wrong by an arcminute.
char
x_ima_b6
The X position of the source in the soft band image in image pixels. (0.2-2.0 keV)
pixels
double
x_ima_b7
The X position of the source in the hard band image in image pixels. (2.0-12.0 keV)
pixels
double
x_ima_b8
The X position of the source in the total band image in image pixels. (0.2-12.0 keV)
pixels
double
ximname_b6
The name of the image containing the soft band detection. (0.2-2.0 keV)
char
ximname_b7
The name of the image containing the hard band detection. (2.0-12.0 keV)
char
ximname_b8
The name of the image containing the total band detection. (0.2-12.0 keV)
char
y_ima_b6
The Y position of the source in the soft band image in image pixels. (0.2-2.0 keV)
pixels
double
y_ima_b7
The Y position of the source in the hard band image in image pixels. (2.0-12.0 keV)
pixels
double
y_ima_b8
The Y position of the source in the total band image in image pixels. (0.2-12.0 keV)
pixels
double
name
This is the official name for sources detected in the XMM-Newton slew survey
meta.id;meta.main
char
primary
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
primary
flux_b8
The source flux in the total energy (0.2-12.0 keV)
(10E-12) ergs/s/cm2
double
primary
flux_b8_err
The error on the total band source flux.
(10E-12) ergs/s/cm2
double
primary
flux_b7
The source flux in the hard energy (2.0-12.0 keV)
(10E-12) ergs/s/cm2
double
primary
flux_b7_err
The error on the hard band source flux
(10E-12) ergs/s/cm2
double
primary
flux_b6
The source flux in the total energy (0.2-2.0 keV)
(10E-12) ergs/s/cm2
double
primary
flux_b6_err
The error on the soft band source flux
(10E-12) ergs/s/cm2
double
primary
catalogues.mv_xsa_epic_source_cat_dr11_fdw
bii
Galactic Latitude [degrees]
deg
double
confused
Normally set False, but set True when a given detection has a probability above zero of being associated with two or more distinct sources.
char
date_end
End date of the observation in UTC
char
date_obs
Start date of the observation in UTC
char
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
detid
Detection identifier of the nearest unique 3XMM-DR7 source in OBS_ID
long
dist_nn
The distance to the nearest neighbouring detection given in arcseconds.
double
duration
Exposure on time
int
ep_1_flux
EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_1_flux_err
Error on EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_2_flux
EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
ep_2_flux_err
Error on the EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
ep_3_flux
EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
ep_3_flux_err
Error on the EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
ep_4_flux
EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
ep_4_flux_err
Error on the EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
ep_5_flux
EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
ep_5_flux_err
Error on the EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
ep_8_cts
EPIC source count in the 0.2-12.0 keV band
count
double
ep_8_cts_err
Error on EPIC source count in the 0.2-12.0 keV band
count
double
ep_8_det_ml
EPIC detection maximum likelihood value in the 0.2-12.0 keV band
double
ep_8_flux
EPIC flux in the 0.2-12.0 keV band
erg/cm**2/s
double
ep_8_flux_err
Error on the EPIC flux in the 0.2-12.0 keV band
erg/cm**2/s
double
ep_8_rate
EPIC count rate in the 0.2-12.0 keV band
count/s
double
ep_8_rate_err
Error on the EPIC count rate in the 0.2-12.0 keV band
count/s
double
ep_9_det_ml
EPIC detection maximum likelihood value in the 0.5-4.5 keV band
double
ep_9_flux
EPIC flux in the 0.5-4.5 keV band (XID band)
erg/cm**2/s
double
ep_9_flux_err
Error on the EPIC flux in the 0.5-4.5 keV band (XID band)
erg/cm**2/s
double
ep_9_rate
EPIC count rate in the 0.5-4.5 keV band
count/s
double
ep_9_rate_err
Error on the EPIC count rate in the 0.5-4.5 keV band
count/s
double
ep_extent
Extent radius of a source detected as extended by the SAS task emldetect
arcsec
double
ep_extent_err
Error on the extent radius of a source detected as extended by the SAS task emldetect
arcsec
double
ep_extent_ml
Extent likelihood of a source detected as extended by the SAS task emldetect
double
ep_hr1
EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr1_err
Error on EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr2
EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr2_err
Error on EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr3
EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr3_err
Error on EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr4
EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
ep_hr4_err
Error on EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
epic_source_cat_equatorial_spoint
char
epic_source_cat_fov_scircle
char
epic_source_cat_galactic_spoint
char
epic_source_cat_oid
Internal Identifier
int
ep_ontime
The EPIC ontime value, given in seconds, is the total good exposure time (after GTI filtering)
s
double
iauname
The IAU name assigned to the unique SRCID
char
lii
Galactic Longitude [degrees]
deg
double
m1_1_bg
M1 background map value in the 0.2-0.5 keV band
count/pixel
double
m1_1_det_ml
M1 detection maximum likelihood value in the 0.2-0.5 keV band
double
m1_1_rate
M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_rate_err
Error on M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_vig
M1 Vignetting map value in the 0.2-0.5 KeV band
double
m1_2_bg
M1 background map value in the 0.5-1.0 keV band
count/pixel
double
m1_2_det_ml
M1 detection maximum likelihood value in the 0.5-1.0 keV band
double
m1_2_rate
M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_2_rate_err
Error on M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_3_bg
M1 background map value in the 1.0-2.0 keV band
count/pixel
double
m1_3_det_ml
M1 detection maximum likelihood value in the 1.0-2.0 keV band
double
m1_3_rate
M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_3_rate_err
Error on M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_4_bg
M1 background map value in the 2.0-4.5 keV band
count/pixel
double
m1_4_det_ml
M1 detection maximum likelihood value in the 2.0-4.5 keV band
double
m1_4_rate
M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_4_rate_err
Error on M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_5_bg
M1 background map value in the 4.5-12.0 keV band
count/pixel
double
m1_5_det_ml
M1 detection maximum likelihood value in the 4.5-12.0 keV band
double
m1_5_rate
M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_5_rate_err
Error on M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_8_cts
M1 source count in the 0.2-12.0 keV band
count
double
m1_8_cts_err
Error on M1 source count in the 0.2-12.0 keV band
count
double
m1_8_det_ml
M1 detection maximum likelihood value in the 0.2-12.0 keV band
double
m1_8_rate
M1 count rate in the 0.2-12.0 keV band
counts/s
double
m1_8_rate_err
Error on M1 count rate in the 0.2-12.0 keV band
counts/s
double
m1_filter
M1 filter. The options are Thick, Medium, Thin1, and Open, depending on the efficiency of the optical blocking.
char
m1_flag
MOS1 flag string made of the flags 1-12 (counted from left to right) for the MOS1 source detection.
char
m1_hr1
M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr1_err
Error on M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr2
M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr2_err
Error on M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr3
M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr3_err
Error on M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr4
M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_hr4_err
Error on M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
m1_pileup
Estimate of the pile-up level in EPIC/MOS1
double
m1_submode
M1 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not exposed ('Fast Uncompressed').
char
m1_submode_friendly_name
M1 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not exposed ('Fast Uncompressed').
char
m2_1_bg
M2 background map value in the 0.2-0.5 keV band
count/pixel
double
m2_1_det_ml
M2 detection maximum likelihood value in the 0.2-0.5 keV band
double
m2_1_rate
M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_rate_err
Error on M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_vig
M2 Vignetting map value in the 0.2-0.5 KeV band
double
m2_2_bg
M2 background map value in the 0.5-1.0 keV band
count/pixel
double
m2_2_det_ml
M2 detection maximum likelihood value in the 0.5-1.0 keV band
double
m2_2_rate
M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_2_rate_err
Error on M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_3_bg
M2 background map value in the 1.0-2.0 keV band
count/pixel
double
m2_3_det_ml
M2 detection maximum likelihood value in the 1.0-2.0 keV band
double
m2_3_rate
M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_3_rate_err
Error on M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_4_bg
M2 background map value in the 2.0-4.5 keV band
count/pixel
double
m2_4_det_ml
M2 detection maximum likelihood value in the 2.0-4.5 keV band
double
m2_4_rate
M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_4_rate_err
Error on M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_5_bg
M2 background map value in the 4.5-12.0 keV band
count/pixel
double
m2_5_det_ml
M2 detection maximum likelihood value in the 4.5-12.0 keV band
double
m2_5_rate
M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_5_rate_err
Error on M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_8_cts
M1 source count in the 0.2-12.0 keV band
count
double
m2_8_cts_err
Error on M1 source count in the 0.2-12.0 keV band
count
double
m2_8_det_ml
M2 detection maximum likelihood value in the 0.2-12.0 keV band
double
m2_8_rate
M2 count rate in the 0.2-12.0 keV band
counts/s
double
m2_8_rate_err
Error on M2 count rate in the 0.2-12.0 keV band
counts/s
double
m2_filter
M2 filter. The options are Thick, Medium, Thin1, and Open, depending on the efficiency of the optical blocking.
char
m2_flag
MOS2 flag string made of the flags 1-12 (counted from left to right) for the MOS2 source detection.
char
m2_hr1
M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr1_err
Error on M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr2
M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr2_err
Error on M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr3
M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr3_err
Error on M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr4
M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_hr4_err
Error on M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
m2_pileup
Estimate of the pile-up level in EPIC/MOS2
double
m2_submode
M2 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not e exposed ('Fast Uncompressed').",
char
m2_submode_friendly_name
M2 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not e exposed ('Fast Uncompressed').
char
mjd_start
Modified Julian Date (i.e., JD - 2400000.5) of the start of the observation.
double
mjd_stop
Modified Julian Date (i.e., JD - 2400000.5) of the end of the observation.
double
n_detections
The number of detections of the unique source SRCID used to derive the combined values.
int
npix
Healpix pixel of the center of the observation for nside 256
long
observation_id
The XMM-Newton observation identification.
char
observation_oid
Internal Identifier for OM observation
int
observer
Principal Investigator Name
char
pn_1_bg
PN background map value in the 0.2-0.5 keV band
count/pixel
double
pn_1_det_ml
PN detection maximum likelihood in the (0.2-0.5 keV) band
double
pn_1_rate
PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_rate_err
Error on the PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_vig
PN Vignetting map value in the 0.2-0.5 KeV band
double
pn_2_bg
PN background map value in the 0.5-1.0 keV band
count/pixel
double
pn_2_det_ml
PN detection maximum likelihood in the (0.5-1.0 keV) band
double
pn_2_rate
PN count rate in the 0.5-1.0 keV band
count/s
double
pn_2_rate_err
Error on PN count rate in the 0.5-1.0 keV band
counts/s
double
pn_3_bg
PN background map value in the 1.0-2.0 keV band
count/pixel
double
pn_3_det_ml
PN detection maximum likelihood in the (1.0-2.0 keV) band
double
pn_3_rate
PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_3_rate_err
Error on PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_4_bg
PN background map value in the 2.0-4.5 keV band
count/pixel
double
pn_4_det_ml
PN detection maximum likelihood in the (2.0-4.5 keV) band
double
pn_4_rate
PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_4_rate_err
Error on PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_5_bg
PN background map value in the 4.5-12.0 keV band
count/pixel
double
pn_5_det_ml
PN detection maximum likelihood in the (4.5-12.0 keV) band
double
pn_5_rate
PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_5_rate_err
Error on PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_8_cts
PN source count in the 0.2-12.0 keV band
count
double
pn_8_cts_err
Error on PN source count in the 0.2-12.0 keV band
count
double
pn_8_det_ml
PN detection maximum likelihood in the (0.2-12.0 keV) band
double
pn_8_rate
PN count rate in the 0.2-12.0 keV
counts/s
double
pn_8_rate_err
Error PN count rate in the 0.2-12.0 keV
counts/s
double
pn_filter
PN filter. The options are Thick, Medium, Thin1, Thin2, and Open, depending on the efficiency of the optical blocking.
char
pn_flag
PN flag string made of the flags 1-12 (counted from left to right) for the PN source detection.
char
pn_hr1
PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr1_err
Error on PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr2
PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr2_err
Error on PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr3
PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr3_err
Error on PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr4
PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_hr4_err
Error on PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
pn_pileup
Estimate of the pile-up level in EPIC/pn
double
pn_submode
PN observing mode. The options are full frame mode with the full FOV exposed (in two sub-modes), and large window mode with only parts of the FOV exposed.
char
pn_submode_friendly_name
PN observing mode. The options are full frame mode with the full FOV exposed (in two sub-modes), and large window mode with only parts of the FOV exposed.
char
poserr
Position error of the nearest 3XMM-DR7 source after field rectifications
arcsec
double
ppsver
PPS Version
char
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
radec_err
Radial error on the position, computed as sqrt(ra_err2 + dec_err2), in arcsecs, where ra_err and dec_err are the 1 sigma uncertainties in the RA and DEC coordinates respectively.
arcsec
double
revolut
The XMM-Newton revolution number
char
sc_chi2prob
The chi square probability (based on the null hypothesis) that the unique source SRCID as detected by any of the observations is constant, that is, the minimum value of the EPIC probabilities in each detection, EP
double
sc_det_ml
Total band detection likelihood of a unique source, calculated as the maximum of the likelihoods of all detections of this source
double
sc_ep_1_flux
The mean band 1 flux (0.2 - 0.5 keV) of all the detections of the source SRCID (see EP_1_FLUX) weighted by the errors (EP_1_FLUX_ERR), in erg/cm2/s.]
erg/cm**2/s
double
sc_ep_1_flux_err
Error on the weighted mean band 1 flux in SC_EP_1_FLUX
erg/cm**2/s
double
sc_ep_2_flux
The mean band 2 flux (0.5 - 1.0 keV) of all the detections of the source SRCID (see EP_2_FLUX) weighted by the errors (EP_2_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_2_flux_err
Error on the weighted mean band 2 flux in SC_EP_2_FLUX
erg/cm**2/s
double
sc_ep_3_flux
The mean band 3 flux (1.0 - 2.0 keV) of all the detections of the source SRCID (see EP_3_FLUX) weighted by the errors (EP_3_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_3_flux_err
Error on the weighted mean band 3 flux in SC_EP_3_FLUX
erg/cm**2/s
double
sc_ep_4_flux
The mean band 4 flux (2.0 - 4.5 keV) of all the detections of the source SRCID (see EP_4_FLUX) weighted by the errors (EP_4_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_4_flux_err
Error on the weighted mean band 4 flux in SC_EP_4_FLUX
erg/cm**2/s
double
sc_ep_5_flux
The mean band 5 flux (4.5 - 12 keV) of all the detections of the source SRCID (see EP_5_FLUX) weighted by the errors (EP_5_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_5_flux_err
Error on the weighted mean band 5 flux in SC_EP_5_FLUX
erg/cm**2/s
double
sc_ep_8_flux
The mean total band flux (0.2 - 12 keV) of all the detections of the source SRCID (see EP_8_FLUX) weighted by the errors (EP_8_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_8_flux_err
Error on the weighted mean band 8 flux in SC_EP_8_FLUX
erg/cm**2/s
double
sc_ep_8_fmax
The maximum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmax_err
The error on the maximum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmin
The minimum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmin_err
The error on the minimum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_9_flux
The mean band 9 flux (0.5 - 4.5 keV) of all the detections of the source SRCID (see EP_9_FLUX) weighted by the errors (EP_9_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_9_flux_err
Error on the weighted mean band 9 flux in SC_EP_9_FLUX
erg/cm**2/s
double
sc_extent
The total band extent (arcseconds) of the source SRCID is the weighted average of the EPIC extents of all detection of this source (EP_EXTENT)
arcsec
double
sc_ext_err
error on source extension
arcsec
double
sc_ext_ml
The total band detection likelihood of the extended source SRCID is the largest of the extent likelihoods of all detection of this source (EP_EXTENT_ML)
double
sc_fvar
The fractional excess variance of the unique source. It is the value corresponding to the exposure and instrument that shows the lowest probability of being constant
double
sc_fvarerr
The error on the fractional excess variance of the unique source. It is the value corresponds to the exposure and instrument that shows the lowest probability of being constant .
double
sc_hr1
The mean hardness ratio of the bands 1 and 2 of all the detections of the source SRCID (EP_HR1) weighted by the errors (EP_HR1_ERR).
double
sc_hr1_err
Error on the weighted mean hardness ration in SC_HR1
double
sc_hr2
The mean hardness ratio of the bands 2 and 3 of all the detections of the source SRCID (EP_HR2) weighted by the errors (EP_HR2_ERR).
double
sc_hr2_err
Error on the weighted mean hardness ration in SC_HR2
double
sc_hr3
The mean hardness ratio of the bands 3 and 4 of all the detections of the source SRCID (EP_HR3) weighted by the errors (EP_HR3_ERR).
double
sc_hr3_err
Error on the weighted mean hardness ration in SC_HR3
double
sc_hr4
The mean hardness ratio of the bands 4 and 5 of all the detections of the source SRCID (EP_HR4) weighted by the errors (EP_HR4_ERR)..
double
sc_hr4_err
Error on the weighted mean hardness ration in SC_HR4
double
sc_sum_flag
The summary flag for the unique source SRCID is taken to be the worst flag of all detections of this source (SUM_FLAG).
int
sc_var_flag
The variability flag for the unique source SRCID is set to VAR_FLAG of the most variable detection of this source. Note that where a timeseries is not available or insufficient points are left in the timeseries after applying background flare GTIs, the value is set to NULL or Undefined
char
spectra
boolean
srcid
A unique number assigned to a group of catalogue entries which are assumed to be the same source.
long
src_num
The (decimal) source number in the individual source list for this observation
int
sum_flag
The summary flag of the detection is derived from the EPIC flag.
int
tseries
boolean
catalogues.mv_xsa_epic_source_cat_dr12_fdw
bii
Galactic Latitude [degrees]
deg
double
ccdm1
M1 CCD number in which detection lies.
int
ccdm2
M2 CCD number in which detection lies.
int
ccdpn
PN CCD number in which detection lies.
int
confused
Normally set False, but set True when a given detection has a probability above zero of being associated with two or more distinct sources.
boolean
date_end
End date of the observation in UTC
char
date_obs
Start date of the observation in UTC
char
detid
Detection identifier of the nearest unique 3XMM-DR7 source in OBS_ID
long
dist_nn
The distance to the nearest neighbouring detection given in arcseconds.
double
duration
Exposure on time
int
ep_1_flux
EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_1_flux_err
Error on EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_8_cts
EPIC source count in the 0.2-12.0 keV band
count
double
ep_8_cts_err
Error on EPIC source count in the 0.2-12.0 keV band
count
double
ep_8_det_ml
EPIC detection maximum likelihood value in the 0.2-12.0 keV band
double
ep_8_rate
EPIC count rate in the 0.2-12.0 keV band
count/s
double
ep_8_rate_err
Error on the EPIC count rate in the 0.2-12.0 keV band
count/s
double
ep_9_det_ml
EPIC detection maximum likelihood value in the 0.5-4.5 keV band
double
ep_9_flux
EPIC flux in the 0.5-4.5 keV band (XID band)
erg/cm**2/s
double
ep_9_flux_err
Error on the EPIC flux in the 0.5-4.5 keV band (XID band)
erg/cm**2/s
double
ep_9_rate
EPIC count rate in the 0.5-4.5 keV band
count/s
double
ep_9_rate_err
Error on the EPIC count rate in the 0.5-4.5 keV band
count/s
double
ep_extent
Extent radius of a source detected as extended by the SAS task emldetect
arcsec
double
ep_extent_err
Error on the extent radius of a source detected as extended by the SAS task emldetect
arcsec
double
ep_extent_ml
Extent likelihood of a source detected as extended by the SAS task emldetect
double
ep_hr1
EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr1_err
Error on EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr2
EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr2_err
Error on EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr3
EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr3_err
Error on EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr4
EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
ep_hr4_err
Error on EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
epic_source_cat_equatorial_spoint
Coordinates of the source on the celestial sphere given in RA and DEC (J2000).
char
epic_source_cat_fov_scircle
Circle projected on the surface of the celestial sphere centered at the coordinates of the source given in RA and DEC (J2000) and a given radius of 15 arc min.
char
epic_source_cat_galactic_spoint
Coordinates of the source on the celestial sphere given in latitude and longitude.
char
epic_source_cat_oid
Internal Identifier
int
ep_ontime
The EPIC ontime value, given in seconds, is the total good exposure time (after GTI filtering)
s
double
high_background
The flag is set to True if this detection comes from a field which, during manual screening, was considered to have a high background level which notably impacted on source detection.
boolean
lii
Galactic Longitude [degrees]
deg
double
m1_1_bg
M1 background map value in the 0.2-0.5 keV band
count/pixel
double
m1_1_det_ml
M1 detection maximum likelihood value in the 0.2-0.5 keV band
double
m1_1_rate
M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_rate_err
Error on M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_vig
M1 Vignetting map value in the 0.2-0.5 KeV band
double
m1_2_bg
M1 background map value in the 0.5-1.0 keV band
count/pixel
double
m1_2_det_ml
M1 detection maximum likelihood value in the 0.5-1.0 keV band
double
m1_2_rate
M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_2_rate_err
Error on M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_3_bg
M1 background map value in the 1.0-2.0 keV band
count/pixel
double
m1_3_det_ml
M1 detection maximum likelihood value in the 1.0-2.0 keV band
double
m1_3_rate
M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_3_rate_err
Error on M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_4_bg
M1 background map value in the 2.0-4.5 keV band
count/pixel
double
m1_4_det_ml
M1 detection maximum likelihood value in the 2.0-4.5 keV band
double
m1_4_rate
M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_4_rate_err
Error on M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_5_bg
M1 background map value in the 4.5-12.0 keV band
count/pixel
double
m1_5_det_ml
M1 detection maximum likelihood value in the 4.5-12.0 keV band
double
m1_5_rate
M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_5_rate_err
Error on M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_8_cts
M1 source count in the 0.2-12.0 keV band
count
double
m1_8_cts_err
Error on M1 source count in the 0.2-12.0 keV band
count
double
m1_8_det_ml
M1 detection maximum likelihood value in the 0.2-12.0 keV band
double
m1_8_rate
M1 count rate in the 0.2-12.0 keV band
counts/s
double
m1_8_rate_err
Error on M1 count rate in the 0.2-12.0 keV band
counts/s
double
m1_filter
M1 filter. The options are Thick, Medium, Thin1, and Open, depending on the efficiency of the optical blocking.
char
m1_flag
MOS1 flag string made of the flags 1-12 (counted from left to right) for the MOS1 source detection.
char
m1_hr1
M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr1_err
Error on M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr2
M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr2_err
Error on M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr3
M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr3_err
Error on M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr4
M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_hr4_err
Error on M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
m1_pileup
Estimate of the pile-up level in EPIC/MOS1
double
m1_submode
M1 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not exposed ('Fast Uncompressed').
char
m1_submode_friendly_name
M1 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not exposed ('Fast Uncompressed').
char
m2_1_bg
M2 background map value in the 0.2-0.5 keV band
count/pixel
double
m2_1_det_ml
M2 detection maximum likelihood value in the 0.2-0.5 keV band
double
m2_1_rate
M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_rate_err
Error on M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_vig
M2 Vignetting map value in the 0.2-0.5 KeV band
double
m2_2_bg
M2 background map value in the 0.5-1.0 keV band
count/pixel
double
m2_2_det_ml
M2 detection maximum likelihood value in the 0.5-1.0 keV band
double
m2_2_rate
M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_2_rate_err
Error on M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_3_bg
M2 background map value in the 1.0-2.0 keV band
count/pixel
double
m2_3_det_ml
M2 detection maximum likelihood value in the 1.0-2.0 keV band
double
m2_3_rate
M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_3_rate_err
Error on M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_4_bg
M2 background map value in the 2.0-4.5 keV band
count/pixel
double
m2_4_det_ml
M2 detection maximum likelihood value in the 2.0-4.5 keV band
double
m2_4_rate
M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_4_rate_err
Error on M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_5_bg
M2 background map value in the 4.5-12.0 keV band
count/pixel
double
m2_5_det_ml
M2 detection maximum likelihood value in the 4.5-12.0 keV band
double
m2_5_rate
M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_5_rate_err
Error on M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_8_cts
M1 source count in the 0.2-12.0 keV band
count
double
m2_8_cts_err
Error on M1 source count in the 0.2-12.0 keV band
count
double
m2_8_det_ml
M2 detection maximum likelihood value in the 0.2-12.0 keV band
double
m2_8_rate
M2 count rate in the 0.2-12.0 keV band
counts/s
double
m2_8_rate_err
Error on M2 count rate in the 0.2-12.0 keV band
counts/s
double
m2_filter
M2 filter. The options are Thick, Medium, Thin1, and Open, depending on the efficiency of the optical blocking.
char
m2_flag
MOS2 flag string made of the flags 1-12 (counted from left to right) for the MOS2 source detection.
char
m2_hr1
M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr1_err
Error on M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr2
M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr2_err
Error on M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr3
M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr3_err
Error on M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr4
M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_hr4_err
Error on M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
m2_pileup
Estimate of the pile-up level in EPIC/MOS2
double
m2_submode
M2 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not e exposed ('Fast Uncompressed').",
char
m2_submode_friendly_name
M2 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not e exposed ('Fast Uncompressed').
char
mjd_stop
Modified Julian Date (i.e., JD - 2400000.5) of the end of the observation.
double
n_detections
The number of detections of the unique source SRCID used to derive the combined values.
int
npix
long
observation_id
The XMM-Newton observation identification.
char
observation_oid
Internal Identifier for OM observation
int
pn_1_bg
PN background map value in the 0.2-0.5 keV band
count/pixel
double
pn_1_det_ml
PN detection maximum likelihood in the (0.2-0.5 keV) band
double
pn_1_rate
PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_rate_err
Error on the PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_vig
PN Vignetting map value in the 0.2-0.5 KeV band
double
pn_2_bg
PN background map value in the 0.5-1.0 keV band
count/pixel
double
pn_2_det_ml
PN detection maximum likelihood in the (0.5-1.0 keV) band
double
pn_2_rate
PN count rate in the 0.5-1.0 keV band
count/s
double
pn_2_rate_err
Error on PN count rate in the 0.5-1.0 keV band
counts/s
double
pn_3_bg
PN background map value in the 1.0-2.0 keV band
count/pixel
double
pn_3_det_ml
PN detection maximum likelihood in the (1.0-2.0 keV) band
double
pn_3_rate
PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_3_rate_err
Error on PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_4_bg
PN background map value in the 2.0-4.5 keV band
count/pixel
double
pn_4_det_ml
PN detection maximum likelihood in the (2.0-4.5 keV) band
double
pn_4_rate
PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_4_rate_err
Error on PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_5_bg
PN background map value in the 4.5-12.0 keV band
count/pixel
double
pn_5_det_ml
PN detection maximum likelihood in the (4.5-12.0 keV) band
double
pn_5_rate
PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_5_rate_err
Error on PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_8_cts
PN source count in the 0.2-12.0 keV band
count
double
pn_8_cts_err
Error on PN source count in the 0.2-12.0 keV band
count
double
pn_8_det_ml
PN detection maximum likelihood in the (0.2-12.0 keV) band
double
pn_8_rate
PN count rate in the 0.2-12.0 keV
counts/s
double
pn_8_rate_err
Error PN count rate in the 0.2-12.0 keV
counts/s
double
pn_filter
PN filter. The options are Thick, Medium, Thin1, Thin2, and Open, depending on the efficiency of the optical blocking.
char
pn_flag
PN flag string made of the flags 1-12 (counted from left to right) for the PN source detection.
char
pn_hr1
PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr1_err
Error on PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr2
PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr2_err
Error on PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr3
PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr3_err
Error on PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr4
PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_hr4_err
Error on PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
pn_pileup
Estimate of the pile-up level in EPIC/pn
double
pn_submode
PN observing mode. The options are full frame mode with the full FOV exposed (in two sub-modes), and large window mode with only parts of the FOV exposed.
char
pn_submode_friendly_name
PN observing mode. The options are full frame mode with the full FOV exposed (in two sub-modes), and large window mode with only parts of the FOV exposed.
char
poserr
Position error of the nearest 3XMM-DR7 source after field rectifications
arcsec
double
ppsver
PPS Version
char
radec_err
Radial error on the position, computed as sqrt(ra_err2 + dec_err2), in arcsecs, where ra_err and dec_err are the 1 sigma uncertainties in the RA and DEC coordinates respectively.
arcsec
double
revolut
The XMM-Newton revolution number
char
sc_chi2prob
The chi square probability (based on the null hypothesis) that the unique source SRCID as detected by any of the observations is constant, that is, the minimum value of the EPIC probabilities in each detection, EP
double
sc_det_ml
Total band detection likelihood of a unique source, calculated as the maximum of the likelihoods of all detections of this source
double
sc_ep_1_flux
The mean band 1 flux (0.2 - 0.5 keV) of all the detections of the source SRCID (see EP_1_FLUX) weighted by the errors (EP_1_FLUX_ERR), in erg/cm2/s.]
erg/cm**2/s
double
sc_ep_1_flux_err
Error on the weighted mean band 1 flux in SC_EP_1_FLUX
erg/cm**2/s
double
sc_ep_2_flux
The mean band 2 flux (0.5 - 1.0 keV) of all the detections of the source SRCID (see EP_2_FLUX) weighted by the errors (EP_2_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_2_flux_err
Error on the weighted mean band 2 flux in SC_EP_2_FLUX
erg/cm**2/s
double
sc_ep_3_flux
The mean band 3 flux (1.0 - 2.0 keV) of all the detections of the source SRCID (see EP_3_FLUX) weighted by the errors (EP_3_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_3_flux_err
Error on the weighted mean band 3 flux in SC_EP_3_FLUX
erg/cm**2/s
double
sc_ep_4_flux
The mean band 4 flux (2.0 - 4.5 keV) of all the detections of the source SRCID (see EP_4_FLUX) weighted by the errors (EP_4_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_4_flux_err
Error on the weighted mean band 4 flux in SC_EP_4_FLUX
erg/cm**2/s
double
sc_ep_5_flux
The mean band 5 flux (4.5 - 12 keV) of all the detections of the source SRCID (see EP_5_FLUX) weighted by the errors (EP_5_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_5_flux_err
Error on the weighted mean band 5 flux in SC_EP_5_FLUX
erg/cm**2/s
double
sc_ep_8_flux
The mean total band flux (0.2 - 12 keV) of all the detections of the source SRCID (see EP_8_FLUX) weighted by the errors (EP_8_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_8_flux_err
Error on the weighted mean band 8 flux in SC_EP_8_FLUX
erg/cm**2/s
double
sc_ep_8_fmax
The maximum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmax_err
The error on the maximum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmin
The minimum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmin_err
The error on the minimum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_9_flux
The mean band 9 flux (0.5 - 4.5 keV) of all the detections of the source SRCID (see EP_9_FLUX) weighted by the errors (EP_9_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_9_flux_err
Error on the weighted mean band 9 flux in SC_EP_9_FLUX
erg/cm**2/s
double
sc_extent
The total band extent (arcseconds) of the source SRCID is the weighted average of the EPIC extents of all detection of this source (EP_EXTENT)
arcsec
double
sc_ext_err
error on source extension
arcsec
double
sc_ext_ml
The total band detection likelihood of the extended source SRCID is the largest of the extent likelihoods of all detection of this source (EP_EXTENT_ML)
double
sc_fvar
The fractional excess variance of the unique source. It is the value corresponding to the exposure and instrument that shows the lowest probability of being constant
double
sc_fvarerr
The error on the fractional excess variance of the unique source. It is the value corresponds to the exposure and instrument that shows the lowest probability of being constant .
double
sc_hr1
The mean hardness ratio of the bands 1 and 2 of all the detections of the source SRCID (EP_HR1) weighted by the errors (EP_HR1_ERR).
double
sc_hr1_err
Error on the weighted mean hardness ration in SC_HR1
double
sc_hr2
The mean hardness ratio of the bands 2 and 3 of all the detections of the source SRCID (EP_HR2) weighted by the errors (EP_HR2_ERR).
double
sc_hr2_err
Error on the weighted mean hardness ration in SC_HR2
double
sc_hr3
The mean hardness ratio of the bands 3 and 4 of all the detections of the source SRCID (EP_HR3) weighted by the errors (EP_HR3_ERR).
double
sc_hr3_err
Error on the weighted mean hardness ration in SC_HR3
double
sc_hr4
The mean hardness ratio of the bands 4 and 5 of all the detections of the source SRCID (EP_HR4) weighted by the errors (EP_HR4_ERR)..
double
sc_hr4_err
Error on the weighted mean hardness ration in SC_HR4
double
sc_sum_flag
The summary flag for the unique source SRCID is taken to be the worst flag of all detections of this source (SUM_FLAG).
int
sc_var_flag
The variability flag for the unique source SRCID is set to VAR_FLAG of the most variable detection of this source. Note that where a timeseries is not available or insufficient points are left in the timeseries after applying background flare GTIs, the value is set to NULL or Undefined
boolean
spectra
The flag is set to True if this detection has a spectrum made in at least one exposure.
boolean
srcid
A unique number assigned to a group of catalogue entries which are assumed to be the same source.
long
src_num
The (decimal) source number in the individual source list for this observation
int
sum_flag
The summary flag of the detection is derived from the EPIC flag.
int
tseries
The flag is set to True if this detection has a time series made in at least one exposure.
boolean
iauname
The IAU name assigned to the unique SRCID
meta.id;meta.main
char
primary
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
primary
ep_8_flux
EPIC flux in the 0.2-12.0 keV band
erg/cm**2/s
double
primary
ep_8_flux_err
Error on the EPIC flux in the 0.2-12.0 keV band
erg/cm**2/s
double
primary
ep_2_flux
EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
primary
ep_2_flux_err
Error on the EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
primary
ep_3_flux
EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
primary
ep_3_flux_err
Error on the EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
primary
ep_4_flux
EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
primary
ep_4_flux_err
Error on the EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
primary
ep_5_flux
EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
primary
ep_5_flux_err
Error on the EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
primary
mjd_start
Modified Julian Date (i.e., JD - 2400000.5) of the start of the observation.
double
primary
catalogues.mv_xsa_epic_source_cat_fdw
The XMM-Newton Serendipitous Source Catalogue: 4XMM-DR14
bii
Galactic Latitude [degrees]
deg
double
ccdm1
M1 CCD number in which detection lies.
int
ccdm2
M2 CCD number in which detection lies.
int
ccdpn
PN CCD number in which detection lies.
int
confused
Normally set False, but set True when a given detection has a probability above zero of being associated with two or more distinct sources.
boolean
date_end
End date of the observation in UTC
char
date_obs
Start date of the observation in UTC
char
dist_nn
The distance to the nearest neighbouring detection given in arcseconds.
double
duration
Exposure on time
int
ep_1_flux
EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_1_flux_err
Error on EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_8_cts
EPIC source count in the 0.2-12.0 keV band
count
double
ep_8_cts_err
Error on EPIC source count in the 0.2-12.0 keV band
count
double
ep_8_det_ml
EPIC detection maximum likelihood value in the 0.2-12.0 keV band
double
ep_8_rate
EPIC count rate in the 0.2-12.0 keV band
count/s
double
ep_8_rate_err
Error on the EPIC count rate in the 0.2-12.0 keV band
count/s
double
ep_9_det_ml
EPIC detection maximum likelihood value in the 0.5-4.5 keV band
double
ep_9_flux
EPIC flux in the 0.5-4.5 keV band (XID band)
erg/cm**2/s
double
ep_9_flux_err
Error on the EPIC flux in the 0.5-4.5 keV band (XID band)
erg/cm**2/s
double
ep_9_rate
EPIC count rate in the 0.5-4.5 keV band
count/s
double
ep_9_rate_err
Error on the EPIC count rate in the 0.5-4.5 keV band
count/s
double
ep_extent
Extent radius of a source detected as extended by the SAS task emldetect
arcsec
double
ep_extent_err
Error on the extent radius of a source detected as extended by the SAS task emldetect
arcsec
double
ep_extent_ml
Extent likelihood of a source detected as extended by the SAS task emldetect
double
ep_hr1
EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr1_err
Error on EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr2
EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr2_err
Error on EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr3
EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr3_err
Error on EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr4
EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
ep_hr4_err
Error on EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
epic_source_cat_equatorial_spoint
Coordinates of the source on the celestial sphere given in RA and DEC (J2000).
char
epic_source_cat_fov_scircle
Circle projected on the surface of the celestial sphere centered at the coordinates of the source given in RA and DEC (J2000) and a given radius of 15 arc min.
char
epic_source_cat_galactic_spoint
Coordinates of the source on the celestial sphere given in latitude and longitude.
char
epic_source_cat_oid
Internal Identifier
int
ep_ontime
The EPIC ontime value, given in seconds, is the total good exposure time (after GTI filtering)
s
double
high_background
The flag is set to True if this detection comes from a field which, during manual screening, was considered to have a high background level which notably impacted on source detection.
boolean
lii
Galactic Longitude [degrees]
deg
double
m1_1_bg
M1 background map value in the 0.2-0.5 keV band
count/pixel
double
m1_1_det_ml
M1 detection maximum likelihood value in the 0.2-0.5 keV band
double
m1_1_rate
M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_rate_err
Error on M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_vig
M1 Vignetting map value in the 0.2-0.5 KeV band
double
m1_2_bg
M1 background map value in the 0.5-1.0 keV band
count/pixel
double
m1_2_det_ml
M1 detection maximum likelihood value in the 0.5-1.0 keV band
double
m1_2_rate
M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_2_rate_err
Error on M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_3_bg
M1 background map value in the 1.0-2.0 keV band
count/pixel
double
m1_3_det_ml
M1 detection maximum likelihood value in the 1.0-2.0 keV band
double
m1_3_rate
M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_3_rate_err
Error on M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_4_bg
M1 background map value in the 2.0-4.5 keV band
count/pixel
double
m1_4_det_ml
M1 detection maximum likelihood value in the 2.0-4.5 keV band
double
m1_4_rate
M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_4_rate_err
Error on M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_5_bg
M1 background map value in the 4.5-12.0 keV band
count/pixel
double
m1_5_det_ml
M1 detection maximum likelihood value in the 4.5-12.0 keV band
double
m1_5_rate
M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_5_rate_err
Error on M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_8_cts
M1 source count in the 0.2-12.0 keV band
count
double
m1_8_cts_err
Error on M1 source count in the 0.2-12.0 keV band
count
double
m1_8_det_ml
M1 detection maximum likelihood value in the 0.2-12.0 keV band
double
m1_8_rate
M1 count rate in the 0.2-12.0 keV band
counts/s
double
m1_8_rate_err
Error on M1 count rate in the 0.2-12.0 keV band
counts/s
double
m1_flag
MOS1 flag string made of the flags 1-12 (counted from left to right) for the MOS1 source detection.
char
m1_hr1
M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr1_err
Error on M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr2
M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr2_err
Error on M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr3
M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr3_err
Error on M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr4
M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_hr4_err
Error on M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
m1_pileup
Estimate of the pile-up level in EPIC/MOS1
double
m1_submode
M1 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not exposed ('Fast Uncompressed').
char
m1_submode_friendly_name
M1 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not exposed ('Fast Uncompressed').
char
m2_1_bg
M2 background map value in the 0.2-0.5 keV band
count/pixel
double
m2_1_det_ml
M2 detection maximum likelihood value in the 0.2-0.5 keV band
double
m2_1_rate
M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_rate_err
Error on M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_vig
M2 Vignetting map value in the 0.2-0.5 KeV band
double
m2_2_bg
M2 background map value in the 0.5-1.0 keV band
count/pixel
double
m2_2_det_ml
M2 detection maximum likelihood value in the 0.5-1.0 keV band
double
m2_2_rate
M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_2_rate_err
Error on M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_3_bg
M2 background map value in the 1.0-2.0 keV band
count/pixel
double
m2_3_det_ml
M2 detection maximum likelihood value in the 1.0-2.0 keV band
double
m2_3_rate
M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_3_rate_err
Error on M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_4_bg
M2 background map value in the 2.0-4.5 keV band
count/pixel
double
m2_4_det_ml
M2 detection maximum likelihood value in the 2.0-4.5 keV band
double
m2_4_rate
M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_4_rate_err
Error on M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_5_bg
M2 background map value in the 4.5-12.0 keV band
count/pixel
double
m2_5_det_ml
M2 detection maximum likelihood value in the 4.5-12.0 keV band
double
m2_5_rate
M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_5_rate_err
Error on M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_8_cts
M1 source count in the 0.2-12.0 keV band
count
double
m2_8_cts_err
Error on M1 source count in the 0.2-12.0 keV band
count
double
m2_8_det_ml
M2 detection maximum likelihood value in the 0.2-12.0 keV band
double
m2_8_rate
M2 count rate in the 0.2-12.0 keV band
counts/s
double
m2_8_rate_err
Error on M2 count rate in the 0.2-12.0 keV band
counts/s
double
m2_flag
MOS2 flag string made of the flags 1-12 (counted from left to right) for the MOS2 source detection.
char
m2_hr1
M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr1_err
Error on M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr2
M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr2_err
Error on M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr3
M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr3_err
Error on M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr4
M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_hr4_err
Error on M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
m2_pileup
Estimate of the pile-up level in EPIC/MOS2
double
m2_submode
M2 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not e exposed ('Fast Uncompressed').,
char
m2_submode_friendly_name
M2 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not e exposed ('Fast Uncompressed').
char
mjd_stop
Modified Julian Date (i.e., JD - 2400000.5) of the end of the observation.
double
n_detections
The number of detections of the unique source SRCID used to derive the combined values.
int
npix
int
observation_id
The XMM-Newton observation identification.
char
observation_oid
Internal Identifier for OM observation
int
pn_1_bg
PN background map value in the 0.2-0.5 keV band
count/pixel
double
pn_1_det_ml
PN detection maximum likelihood in the (0.2-0.5 keV) band
double
pn_1_rate
PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_rate_err
Error on the PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_vig
PN Vignetting map value in the 0.2-0.5 KeV band
double
pn_2_bg
PN background map value in the 0.5-1.0 keV band
count/pixel
double
pn_2_det_ml
PN detection maximum likelihood in the (0.5-1.0 keV) band
double
pn_2_rate
PN count rate in the 0.5-1.0 keV band
count/s
double
pn_2_rate_err
Error on PN count rate in the 0.5-1.0 keV band
counts/s
double
pn_3_bg
PN background map value in the 1.0-2.0 keV band
count/pixel
double
pn_3_det_ml
PN detection maximum likelihood in the (1.0-2.0 keV) band
double
pn_3_rate
PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_3_rate_err
Error on PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_4_bg
PN background map value in the 2.0-4.5 keV band
count/pixel
double
pn_4_det_ml
PN detection maximum likelihood in the (2.0-4.5 keV) band
double
pn_4_rate
PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_4_rate_err
Error on PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_5_bg
PN background map value in the 4.5-12.0 keV band
count/pixel
double
pn_5_det_ml
PN detection maximum likelihood in the (4.5-12.0 keV) band
double
pn_5_rate
PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_5_rate_err
Error on PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_8_cts
PN source count in the 0.2-12.0 keV band
count
double
pn_8_cts_err
Error on PN source count in the 0.2-12.0 keV band
count
double
pn_8_det_ml
PN detection maximum likelihood in the (0.2-12.0 keV) band
double
pn_8_rate
PN count rate in the 0.2-12.0 keV
counts/s
double
pn_8_rate_err
Error PN count rate in the 0.2-12.0 keV
counts/s
double
pn_flag
PN flag string made of the flags 1-12 (counted from left to right) for the PN source detection.
char
pn_hr1
PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr1_err
Error on PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr2
PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr2_err
Error on PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr3
PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr3_err
Error on PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr4
PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_hr4_err
Error on PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_offax
Distance between the detection position and the onaxis position on the respective detector.
arcmin
double
pn_pileup
Estimate of the pile-up level in EPIC/pn
double
pn_submode
PN observing mode. The options are full frame mode with the full FOV exposed (in two sub-modes), and large window mode with only parts of the FOV exposed.
char
pn_submode_friendly_name
PN observing mode. The options are full frame mode with the full FOV exposed (in two sub-modes), and large window mode with only parts of the FOV exposed.
char
poserr
Position error of the nearest 3XMM-DR7 source after field rectifications
arcsec
double
ppsver
PPS Version
char
radec_err
Radial error on the position, computed as sqrt(ra_err2 + dec_err2), in arcsecs, where ra_err and dec_err are the 1 sigma uncertainties in the RA and DEC coordinates respectively.
arcsec
double
revolut
The XMM-Newton revolution number
char
sc_chi2prob
The chi square probability (based on the null hypothesis) that the unique source SRCID as detected by any of the observations is constant, that is, the minimum value of the EPIC probabilities in each detection, EP
double
sc_det_ml
Total band detection likelihood of a unique source, calculated as the maximum of the likelihoods of all detections of this source
double
sc_ep_1_flux
The mean band 1 flux (0.2 - 0.5 keV) of all the detections of the source SRCID (see EP_1_FLUX) weighted by the errors (EP_1_FLUX_ERR), in erg/cm2/s.]
erg/cm**2/s
double
sc_ep_1_flux_err
Error on the weighted mean band 1 flux in SC_EP_1_FLUX
erg/cm**2/s
double
sc_ep_2_flux
The mean band 2 flux (0.5 - 1.0 keV) of all the detections of the source SRCID (see EP_2_FLUX) weighted by the errors (EP_2_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_2_flux_err
Error on the weighted mean band 2 flux in SC_EP_2_FLUX
erg/cm**2/s
double
sc_ep_3_flux
The mean band 3 flux (1.0 - 2.0 keV) of all the detections of the source SRCID (see EP_3_FLUX) weighted by the errors (EP_3_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_3_flux_err
Error on the weighted mean band 3 flux in SC_EP_3_FLUX
erg/cm**2/s
double
sc_ep_4_flux
The mean band 4 flux (2.0 - 4.5 keV) of all the detections of the source SRCID (see EP_4_FLUX) weighted by the errors (EP_4_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_4_flux_err
Error on the weighted mean band 4 flux in SC_EP_4_FLUX
erg/cm**2/s
double
sc_ep_5_flux
The mean band 5 flux (4.5 - 12 keV) of all the detections of the source SRCID (see EP_5_FLUX) weighted by the errors (EP_5_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_5_flux_err
Error on the weighted mean band 5 flux in SC_EP_5_FLUX
erg/cm**2/s
double
sc_ep_8_flux
The mean total band flux (0.2 - 12 keV) of all the detections of the source SRCID (see EP_8_FLUX) weighted by the errors (EP_8_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_8_flux_err
Error on the weighted mean band 8 flux in SC_EP_8_FLUX
erg/cm**2/s
double
sc_ep_8_fmax
The maximum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmax_err
The error on the maximum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmin
The minimum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_8_fmin_err
The error on the minimum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source.
erg/cm**2/s
double
sc_ep_9_flux
The mean band 9 flux (0.5 - 4.5 keV) of all the detections of the source SRCID (see EP_9_FLUX) weighted by the errors (EP_9_FLUX_ERR), in erg/cm2/s.
erg/cm**2/s
double
sc_ep_9_flux_err
Error on the weighted mean band 9 flux in SC_EP_9_FLUX
erg/cm**2/s
double
sc_extent
The total band extent (arcseconds) of the source SRCID is the weighted average of the EPIC extents of all detection of this source (EP_EXTENT)
arcsec
double
sc_ext_err
error on source extension
arcsec
double
sc_ext_ml
The total band detection likelihood of the extended source SRCID is the largest of the extent likelihoods of all detection of this source (EP_EXTENT_ML)
double
sc_fvar
The fractional excess variance of the unique source. It is the value corresponding to the exposure and instrument that shows the lowest probability of being constant
double
sc_fvarerr
The error on the fractional excess variance of the unique source. It is the value corresponds to the exposure and instrument that shows the lowest probability of being constant .
double
sc_hr1
The mean hardness ratio of the bands 1 and 2 of all the detections of the source SRCID (EP_HR1) weighted by the errors (EP_HR1_ERR).
double
sc_hr1_err
Error on the weighted mean hardness ration in SC_HR1
double
sc_hr2
The mean hardness ratio of the bands 2 and 3 of all the detections of the source SRCID (EP_HR2) weighted by the errors (EP_HR2_ERR).
double
sc_hr2_err
Error on the weighted mean hardness ration in SC_HR2
double
sc_hr3
The mean hardness ratio of the bands 3 and 4 of all the detections of the source SRCID (EP_HR3) weighted by the errors (EP_HR3_ERR).
double
sc_hr3_err
Error on the weighted mean hardness ration in SC_HR3
double
sc_hr4
The mean hardness ratio of the bands 4 and 5 of all the detections of the source SRCID (EP_HR4) weighted by the errors (EP_HR4_ERR)..
double
sc_hr4_err
Error on the weighted mean hardness ration in SC_HR4
double
sc_sum_flag
The summary flag for the unique source SRCID is taken to be the worst flag of all detections of this source (SUM_FLAG).
int
sc_var_flag
The variability flag for the unique source SRCID is set to VAR_FLAG of the most variable detection of this source. Note that where a timeseries is not available or insufficient points are left in the timeseries after applying background flare GTIs, the value is set to NULL or Undefined
boolean
spectra
The flag is set to True if this detection has a spectrum made in at least one exposure.
boolean
srcid
A unique number assigned to a group of catalogue entries which are assumed to be the same source.
long
src_num
The (decimal) source number in the individual source list for this observation
int
sum_flag
The summary flag of the detection is derived from the EPIC flag.
int
iauname
The IAU name assigned to the unique SRCID
char
primary
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
primary
detid
Detection identifier of the nearest unique 3XMM-DR7 source in OBS_ID
meta.id;meta.main
long
primary
ep_8_flux
EPIC flux in the 0.2-12.0 keV band
erg/cm**2/s
double
primary
ep_8_flux_err
Error on the EPIC flux in the 0.2-12.0 keV band
erg/cm**2/s
double
primary
ep_2_flux
EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
primary
ep_2_flux_err
Error on the EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
primary
ep_3_flux
EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
primary
ep_3_flux_err
Error on the EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
primary
ep_4_flux
EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
primary
ep_4_flux_err
Error on the EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
primary
ep_5_flux
EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
primary
ep_5_flux_err
Error on the EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
primary
mjd_start
Modified Julian Date (i.e., JD - 2400000.5) of the start of the observation.
double
primary
m1_filter
M1 filter. The options are Thick, Medium, Thin1, and Open, depending on the efficiency of the optical blocking.
char
primary
m2_filter
M2 filter. The options are Thick, Medium, Thin1, and Open, depending on the efficiency of the optical blocking.
char
primary
pn_filter
PN filter. The options are Thick, Medium, Thin1, Thin2, and Open, depending on the efficiency of the optical blocking.
char
primary
tseries
The flag is set to True if this detection has a time series made in at least one exposure.
boolean
catalogues.mv_xsa_epic_stack_cat_dr11_fdw
astcorr
Flag: observation was astrometrically corrected
boolean
bii
Galactic Latitude [degrees]
deg
double
cc_deofferr
1-sigma error on CC_DEOFFSET
arcsec
double
cc_deoffset
catcorr shift of the declination in the field
arcsec
double
cc_nmatches
catcorr number of usable matches with the reference catalogue
int
cc_pofferr
1-sigma error on CC_POFFSET
arcsec
double
cc_poffset
catcorr total position shift of the field
arcsec
double
cc_raofferr
1-sigma error on CC_RAOFFSET
arcsec
double
cc_raoffset
catcorr shift of the right ascension in the field
arcsec
double
cc_refcat
catcorr reference catalogue
char
cc_rot_corr
catcorr shift of the position angle in the field
deg
double
cc_rot_err
1-sigma error on CC_ROT_CORR
deg
double
chi2prob_4xmmdr11
Probability of the DR7 source to be consistent with constant flux
double
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
dec_4xmmdr11
Mean declination (SC_)DEC of the nearest unique 4XMM-DR11 source
double
detid_4xmmdr11
Detection identifier of the nearest unique 4XMM-DR11 source in OBS_ID
long
dist_4xmmdr11
Distance to the nearest 4XMM-DR11 source / its detection in OBS_ID
double
dist_nn
The distance to the nearest neighbouring detection given in arcseconds.
double
dist_ref
Distance to the reference coordinates of the field
arcmin
double
ep_1_flux
EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_1_flux_err
Error on EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_2_flux
EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
ep_2_flux_err
Error on the EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
ep_3_flux
EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
ep_3_flux_err
Error on the EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
ep_4_flux
EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
ep_4_flux_err
Error on the EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
ep_5_flux
EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
ep_5_flux_err
Error on the EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
ep_cts
All EPIC number of counts
counts
double
ep_cts_err
1-sigma error on EP_CTS
counts
double
ep_det_ml
All-EPIC equivalent maximum detection likelihood
double
ep_flag
EPIC Quality Flag
char
ep_flux
EPIC flux in the 0.2-12.0 keV band
erg/cm²/s
double
ep_flux_err
1-sigma Error on EPIC flux in the 0.2-12.0 keV band
erg/cm²/s
double
ep_hr1
EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr1_err
Error on EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr2
EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr2_err
Error on EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr3
EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr3_err
Error on EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr4
EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
ep_hr4_err
Error on EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
epic_stack_cat_equatorial_spoint
char
epic_stack_cat_fov_scircle
char
epic_stack_cat_galactic_spoint
char
epic_xmm_stack_cat_oid
Internal identifier
int
ep_offax
Minimum EPIC offaxis angle between source position and aim point
arcmin
double
ep_ontime
The EPIC ontime value, given in seconds, is the total good exposure time (after GTI filtering)
s
double
ep_rate
All EPIC count rate
counts/s
double
ep_rate_err
1-sigma error on EP_RATE
counts/s
double
extent
Extent radius
arcsec
double
extent_err
1-sigma error on EXTENT
arcsec
double
extent_ml
Likelihood of the detection being extended
double
fbr_var_chi2_21
Reduced chi square of EPIC band 2 to 1 inter-observation variability
double
fbr_var_chi2_31
Reduced chi square of EPIC band 3 to 1 inter-observation variability
double
fbr_var_chi2_32
Reduced chi square of EPIC band 3 to 2 inter-observation variability
double
fbr_var_chi2_41
Reduced chi square of EPIC band 4 to 1 inter-observation variability
double
fbr_var_chi2_42
Reduced chi square of EPIC band 4 to 2 inter-observation variability
double
fbr_var_chi2_43
Reduced chi square of EPIC band 4 to 3 inter-observation variability
double
fbr_var_chi2_51
Reduced chi square of EPIC band 5 to 1 inter-observation variability
double
fbr_var_chi2_52
Reduced chi square of EPIC band 5 to 2 inter-observation variability
double
fbr_var_chi2_53
Reduced chi square of EPIC band 5 to 3 inter-observation variability
double
fbr_var_chi2_54
Reduced chi square of EPIC band 5 to 4 inter-observation variability
double
fbr_var_dsig_21
Largest difference of EPIC band 2 to 1 flux ratios in terms of sigma
double
fbr_var_dsig_31
Largest difference of EPIC band 3 to 1 flux ratios in terms of sigma
double
fbr_var_dsig_32
Largest difference of EPIC band 3 to 2 flux ratios in terms of sigma
double
fbr_var_dsig_41
Largest difference of EPIC band 4 to 1 flux ratios in terms of sigma
double
fbr_var_dsig_42
Largest difference of EPIC band 4 to 2 flux ratios in terms of sigma
double
fbr_var_dsig_43
Largest difference of EPIC band 4 to 3 flux ratios in terms of sigma
double
fbr_var_dsig_51
Largest difference of EPIC band 5 to 1 flux ratios in terms of sigma
double
fbr_var_dsig_52
Largest difference of EPIC band 5 to 2 flux ratios in terms of sigma
double
fbr_var_dsig_53
Largest difference of EPIC band 5 to 3 flux ratios in terms of sigma
double
fbr_var_dsig_54
Largest difference of EPIC band 5 to 4 flux ratios in terms of sigma
double
fbr_var_prob_21
Probability that the flux band 2 to 1 variability is consistent
double
fbr_var_prob_31
Probability that the flux band 3 to 1 variability is consistent
double
fbr_var_prob_32
Probability that the flux band 3 to 2 variability is consistent
double
fbr_var_prob_41
Probability that the flux band 4 to 1 variability is consistent
double
fbr_var_prob_42
Probability that the flux band 4 to 2 variability is consistent
double
fbr_var_prob_43
Probability that the flux band 4 to 3 variability is consistent
double
fbr_var_prob_51
Probability that the flux band 5 to 1 variability is consistent
double
fbr_var_prob_52
Probability that the flux band 5 to 2 variability is consistent
double
fbr_var_prob_53
Probability that the flux band 5 to 3 variability is consistent
double
fbr_var_prob_54
Probability that the flux band 5 to 4 variability is consistent
double
fluxvar
Largest EPIC flux difference in terms of sigma
double
fluxvar_1
Largest EPIC band 1 flux difference in terms of sigma
double
fluxvar_2
Largest EPIC band 2 flux difference in terms of sigma
double
fluxvar_3
Largest EPIC band 3 flux difference in terms of sigma
double
fluxvar_4
Largest EPIC band 4 flux difference in terms of sigma
double
fluxvar_5
Largest EPIC band 5 flux difference in terms of sigma
double
fratio
EPIC flux ratio
double
fratio_1
EPIC band 1 flux ration
double
fratio_1_err
1-sigma error on F_RATIO_1
double
fratio_2
EPIC band 2 flux ration
double
fratio_2_err
1-sigma error on F_RATIO_2
double
fratio_3
EPIC band 3 flux ration
double
fratio_3_err
1-sigma error on F_RATIO_3
double
fratio_4
EPIC band 4 flux ration
double
fratio_4_err
1-sigma error on F_RATIO_4
double
fratio_5
EPIC band 5 flux ration
double
fratio_5_err
1-sigma error on F_RATIO_5
double
fratio_err
1-sigma error on F_RATIO
double
fvar_4xmmdr11
Fractional intra-obs. excess variance of the nearest 4XMM-DR11 source
double
fvarerr_4xmmdr11
1-sigma error on FVAR_4XMM-DR11
double
iauname
IAU name of the source
char
iauname_4xmmdr11
IAU name assigned to the nearest unique 4XMM-DR11 source
char
lii
Galactic Longitude [degrees]
deg
double
m1_1_bg
M1 background map value in the 0.2-0.5 keV band
count/pixel
double
m1_1_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 1
double
m1_1_exp
PSF-weighted exposure of the detection in energy band 1 on EPIC/MOS1
s
double
m1_1_flux
EPIC/MOS1 Flux in Energy band 1
erg/cm²/s
double
m1_1_flux_err
1-sigma error on M1_2_FLUX
erg/cm²/s
double
m1_1_rate
M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_rate_err
Error on M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_vig
M1 Vignetting map value in the 0.2-0.5 KeV band
double
m1_2_bg
M1 background map value in the 0.5-1.0 keV band
count/pixel
double
m1_2_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 2
double
m1_2_exp
PSF-weighted exposure of the detection in energy band 2 on EPIC/MOS1
s
double
m1_2_flux
EPIC/MOS1 Flux in Energy band 2
erg/cm²/s
double
m1_2_flux_err
1-sigma error on M1_3_FLUX
erg/cm²/s
double
m1_2_rate
M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_2_rate_err
Error on M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_2_vig
EPIC/MOS1 vignetting factor in energy band 1 for the observation
double
m1_3_bg
M1 background map value in the 1.0-2.0 keV band
count/pixel
double
m1_3_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 3
double
m1_3_exp
PSF-weighted exposure of the detection in energy band 3 on EPIC/MOS1
s
double
m1_3_flux
EPIC/MOS1 Flux in Energy band 3
erg/cm²/s
double
m1_3_flux_err
1-sigma error on M1_4_FLUX
erg/cm²/s
double
m1_3_rate
M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_3_rate_err
Error on M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_3_vig
EPIC/MOS1 vignetting factor in energy band 2 for the observation
double
m1_4_bg
M1 background map value in the 2.0-4.5 keV band
count/pixel
double
m1_4_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 4
double
m1_4_exp
PSF-weighted exposure of the detection in energy band 4 on EPIC/MOS1
s
double
m1_4_flux
EPIC/MOS1 Flux in Energy band 3
erg/cm²/s
double
m1_4_flux_err
1-sigma error on M1_4_FLUX
erg/cm²/s
double
m1_4_rate
M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_4_rate_err
Error on M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_4_vig
EPIC/MOS1 vignetting factor in energy band 3 for the observation
double
m1_5_bg
M1 background map value in the 4.5-12.0 keV band
count/pixel
double
m1_5_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 5
double
m1_5_exp
PSF-weighted exposure of the detection in energy band 5 on EPIC/MOS1
s
double
m1_5_flux
EPIC/MOS1 Flux in Energy band 5
erg/cm²/s
double
m1_5_flux_err
1-sigma error on M1_5_FLUX
erg/cm²/s
double
m1_5_rate
M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_5_rate_err
Error on M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_5_vig
EPIC/MOS1 vignetting factor in energy band 5 for the observation
double
m1_bg
EPIC/MOS1 background map at detection position
counts/pixel
double
m1_bkg_cprob
EPIC/MOS1 Cauchy probability derived from M1_BKG_CRAREA
double
m1_bkg_crarea
EPIC/MOS1 background rate per area
counts/s/arcsec2
double
m1_cts
EPIC MOS1 number of counts
counts
double
m1_cts_err
1-sigma error on M1_CTS
counts
double
m1_det_ml
EPIC/MOS1 equ. maximum detection likelihood.
double
m1_exp
PSF-weighted exposure of the detection in EPIC/MOS1
s
double
m1_filter
M1 filter. The options are Thick, Medium, Thin1, and Open, depending on the efficiency of the optical blocking.
char
m1_flag
MOS1 flag string made of the flags 1-12 (counted from left to right) for the MOS1 source detection.
char
m1_flux
Total EPIC/MOS1 flux
erg/cm²/s
double
m1_flux_err
1-sigma error on M1_1_FLUX
erg/cm²/s
double
m1_hr1
M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr1_err
Error on M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr2
M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr2_err
Error on M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr3
M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr3_err
Error on M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr4
M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_hr4_err
Error on M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_maskfrac
PSF-weighted detector coverage in EPIC/M1
double
m1_offax
Distance between the detector position and the onaxis position on the respective detector.
arcmin
double
m1_ontime
Total good exposure time in EPIC/MOS1
s
double
m1_pileup
Estimate of the pile-up level in EPIC/MOS1
double
m1_rate
Total EPIC/MOS1 count rate
counts/s
double
m1_rate_err
1-sigma error on M1_RATE
counts/s
double
m1_submode
M1 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not exposed ('Fast Uncompressed').
char
m2_1_bg
M2 background map value in the 0.2-0.5 keV band
count/pixel
double
m2_1_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 1
double
m2_1_exp
PSF-weighted exposure of the detection in energy band 1 on EPIC/MOS2
s
double
m2_1_flux
EPIC/MOS2 Flux in Energy band 1
erg/cm²/s
double
m2_1_flux_err
1-sigma error on M2_1_FLUX
erg/cm²/s
double
m2_1_rate
M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_rate_err
Error on M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_vig
M2 Vignetting map value in the 0.2-0.5 KeV band
double
m2_2_bg
M2 background map value in the 0.5-1.0 keV band
count/pixel
double
m2_2_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 2
double
m2_2_exp
PSF-weighted exposure of the detection in energy band 2 on EPIC/MOS2
s
double
m2_2_flux
EPIC/MOS2 Flux in Energy band 2
erg/cm²/s
double
m2_2_flux_err
1-sigma error on M2_2_FLUX
erg/cm²/s
double
m2_2_rate
M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_2_rate_err
Error on M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_2_vig
EPIC/MOS2 vignetting factor in energy band 2 for the observation
double
m2_3_bg
M2 background map value in the 1.0-2.0 keV band
count/pixel
double
m2_3_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 3
double
m2_3_exp
PSF-weighted exposure of the detection in energy band 3 on EPIC/MOS2
s
double
m2_3_flux
EPIC/MOS2 Flux in Energy band 3
erg/cm²/s
double
m2_3_flux_err
1-sigma error on M2_3_FLUX
erg/cm²/s
double
m2_3_rate
M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_3_rate_err
Error on M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_3_vig
EPIC/MOS2 vignetting factor in energy band 3 for the observation
double
m2_4_bg
M2 background map value in the 2.0-4.5 keV band
count/pixel
double
m2_4_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 4
double
m2_4_exp
PSF-weighted exposure of the detection in energy band 4 on EPIC/MOS2
s
double
m2_4_flux
EPIC/MOS2 Flux in Energy band 4
erg/cm²/s
double
m2_4_flux_err
1-sigma error on M2_4_FLUX
erg/cm²/s
double
m2_4_rate
M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_4_rate_err
Error on M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_4_vig
EPIC/MOS2 vignetting factor in energy band 4 for the observation
double
m2_5_bg
M2 background map value in the 4.5-12.0 keV band
count/pixel
double
m2_5_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 5
double
m2_5_exp
PSF-weighted exposure of the detection in energy band 5 on EPIC/MOS2
s
double
m2_5_flux
EPIC/MOS2 Flux in Energy band 5
erg/cm²/s
double
m2_5_flux_err
1-sigma error on M2_5_FLUX
erg/cm²/s
double
m2_5_rate
M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_5_rate_err
Error on M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_5_vig
EPIC/MOS2 vignetting factor in energy band 5 for the observation
double
m2_bg
EPIC/MOS2 background map at detection position
counts/pixel
double
m2_bkg_cprob
EPIC/MOS2 Cauchy probability derived from M2_BKG_CRAREA
double
m2_bkg_crarea
EPIC/MOS2 background rate per area
counts/s/arcsec2
double
m2_cts
EPIC MOS2 number of counts
counts
double
m2_cts_err
1-sigma error on M2_CTS
counts
double
m2_det_ml
EPIC/MOS2 equ. maximum detection likelihood.
double
m2_exp
PSF-weighted exposure of the detection in EPIC/MOS1
s
double
m2_filter
M2 filter. The options are Thick, Medium, Thin1, and Open, depending on the efficiency of the optical blocking.
char
m2_flag
MOS2 flag string made of the flags 1-12 (counted from left to right) for the MOS2 source detection.
char
m2_flux
Total EPIC/MOS2 flux
erg/cm²/s
double
m2_flux_err
1-sigma error on M2_FLUX
erg/cm²/s
double
m2_hr1
M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr1_err
Error on M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr2
M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr2_err
Error on M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr3
M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr3_err
Error on M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr4
M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_hr4_err
Error on M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_maskfrac
PSF-weighted detector coverage in EPIC/M2
double
m2_offax
Distance between the detector position and the onaxis position on the respective detector.
arcmin
double
m2_ontime
Total good exposure time in EPIC/MOS2
s
double
m2_pileup
Estimate of the pile-up level in EPIC/MOS2
double
m2_rate
EPIC/MOS2 count rate .
counts/s
double
m2_rate_err
1-sigma error on M2_RATE
counts/s
double
m2_submode
M2 observing mode. The options are full frame mode with the full FOV exposed, partial window mode with only parts of the central CCD exposed and timing mode where the central CCD was not e exposed ('Fast Uncompressed').",
char
mjd_first
Modified Julian DATE JD-2400000.5 of the observation start
d
double
mjd_last
Modified Julian DATE JD-2400000.5 of the observation end
d
double
n_blend
Number of simultaneously fit sources
int
n_contrib
Number of pointings in which the source was fitted
pixel
int
ndetect_4xmmdr11
Number of DR7 detections of the nearest unique 4XMM-DR11 source
int
n_exp
Number of instruments for which the source was fitted
int
n_obs
Number of observations involved in the stack
int
npix
Healpix pixel of the center of the observation for nside 256
long
obs_class
Observation quality from 4XMM-DR11 screening
int
obs_id
XMM-Newton observation identification
char
overlap
Flag: observation was astrometrically corrected
boolean
pa_pnt
Mean position angle of the spacecraft
deg
double
pn_1_bg
PN background map value in the 0.2-0.5 keV band
count/pixel
double
pn_1_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 1
double
pn_1_exp
PSF-weighted exposure of the detection in energy band 1 on EPIC/PN
s
double
pn_1_flux
EPIC/PN flux on energy band 1
erg/cm²/s
double
pn_1_flux_err
1-sigma error on PN_FLUX_1
erg/cm²/s
double
pn_1_rate
PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_rate_err
Error on the PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_vig
PN Vignetting map value in the 0.2-0.5 KeV band
double
pn_2_bg
PN background map value in the 0.5-1.0 keV band
count/pixel
double
pn_2_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 2
double
pn_2_exp
PSF-weighted exposure of the detection in energy band 2 on EPIC/PN
s
double
pn_2_flux
EPIC/PN flux on energy band 2
erg/cm²/s
double
pn_2_flux_err
1-sigma error on PN_FLUX_2
erg/cm²/s
double
pn_2_rate
PN count rate in the 0.5-1.0 keV band
count/s
double
pn_2_rate_err
Error on PN count rate in the 0.5-1.0 keV band
counts/s
double
pn_2_vig
EPIC/PN vignetting factor in energy band 2 for the observation
double
pn_3_bg
PN background map value in the 1.0-2.0 keV band
count/pixel
double
pn_3_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 3
double
pn_3_exp
PSF-weighted exposure of the detection in energy band 3 on EPIC/PN
s
double
pn_3_flux
EPIC/PN flux on energy band 3
erg/cm²/s
double
pn_3_flux_err
1-sigma error on PN_FLUX_3
erg/cm²/s
double
pn_3_rate
PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_3_rate_err
Error on PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_3_vig
EPIC/PN vignetting factor in energy band 3 for the observation
double
pn_4_bg
PN background map value in the 2.0-4.5 keV band
count/pixel
double
pn_4_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 4
double
pn_4_exp
PSF-weighted exposure of the detection in energy band 4 on EPIC/PN
s
double
pn_4_flux
EPIC/PN flux on energy band 4
erg/cm²/s
double
pn_4_flux_err
1-sigma error on PN_FLUX_4
erg/cm²/s
double
pn_4_rate
PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_4_rate_err
Error on PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_4_vig
EPIC/PN vignetting factor in energy band 4 for the observation
double
pn_5_bg
PN background map value in the 4.5-12.0 keV band
count/pixel
double
pn_5_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 5.
double
pn_5_exp
PSF-weighted exposure of the detection in energy band 5 on EPIC/PN
s
double
pn_5_flux
EPIC/PN Flux in Energy band 5
erg/cm²/s
double
pn_5_flux_err
1-sigma error on PN_5_FLUX
erg/cm²/s
double
pn_5_rate
PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_5_rate_err
Error on PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_5_vig
EPIC/PN vignetting factor in energy band 5 for the observation
double
pn_bg
EPIC/PN background map at detection position
counts/pixel
double
pn_bkg_cprob
EPIC/pn Cauchy probability derived from PN_BKG_CRAREA
double
pn_bkg_crarea
EPIC/pn background rate per area
counts/s/arcsec2
double
pn_cts
EPIC PN number of counts
counts
double
pn_cts_err
1-sigma error on PN_CTS
counts
double
pn_det_ml
EPIC/PN equ. maximum detection likelihood
double
pn_exp
PSF-weighted exposure of the detection in EPIC/PN
s
double
pn_filter
PN filter. The options are Thick, Medium, Thin1, Thin2, and Open, depending on the efficiency of the optical blocking.
char
pn_flag
PN flag string made of the flags 1-12 (counted from left to right) for the PN source detection.
char
pn_flux
Total EPIC/pn flux
erg/cm²/s
double
pn_flux_err
1-sigma error on PN_FLUX
erg/cm²/s
double
pn_hr1
PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr1_err
Error on PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr2
PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr2_err
Error on PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr3
PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr3_err
Error on PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr4
PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_hr4_err
Error on PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_maskfrac
PSF-weighted detector coverage in EPIC/PN
double
pn_offax
Distance between the detector position and the onaxis position on the respective detector.
arcmin
double
pn_ontime
Total good exposure time all-EPIC
s
double
pn_pileup
Estimate of the pile-up level in EPIC/pn
double
pn_rate
Total EPIC/pn count rate
counts/s
double
pn_rate_err
1-sigma error on PN_RATE
counts/s
double
pn_submode
PN observing mode. The options are full frame mode with the full FOV exposed (in two sub-modes), and large window mode with only parts of the FOV exposed.
char
poserr_4xmmdr11
Statistical & systematic position error of the 4XMM-DR11 source
double
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
ra_4xmmdr11
Mean right ascension (SC_)RA of the nearest unique 4XMM-DR11 source
double
radec_err
Radial error on the position, computed as sqrt(ra_err2 + dec_err2), in arcsecs, where ra_err and dec_err are the 1 sigma uncertainties in the RA and DEC coordinates respectively.
double
revolut
The XMM-Newton revolution number
orbit
int
srcid
A unique number assigned to a group of catalogue entries which are assumed to be the same source.
long
srcid_4xmmdr11
Source identifier of the nearest unique source in 4XMM-DR11
long
stack_flag
Integer representation of the stack detection flags
int
sum_flag_4xmmdr11
Summary quality flag of the nearest unique 4XMM-DR11 source
int
sum_flag_min_4xmmdr11
Best quality flag of the detections of the nearest 4XMM-DR11 source
int
url_4xmmdr11
Webpage URL of the nearest 4XMM-DR11 source
char
var_chi2
Reduced chi-square of EPIC inter-observation variability.
double
var_chi2_1
Reduced chi-square of EPIC band 1 inter-observation variability.
double
var_chi2_2
Reduced chi-square of EPIC band 2 inter-observation variability.
double
var_chi2_3
Reduced chi-square of EPIC band 3 inter-observation variability.
double
var_chi2_4
Reduced chi-square of EPIC band 4 inter-observation variability.
double
var_chi2_5
Reduced chi-square of EPIC band 5 inter-observation variability.
double
var_flag_4xmmdr11
Intra-observation variability flag of the nearest 4XMM-DR11 source
boolean
var_prob
Probability to be consistent with constant flux from VAR_CHI2
double
var_prob_1
Band 1 Probability to be consistent with constant flux from VAR_CHI2_1
double
var_prob_2
Band 2 Probability to be consistent with constant flux from VAR_CHI2_2
double
var_prob_3
Band 3 Probability to be consistent with constant flux from VAR_CHI2_3
double
var_prob_4
Band 4 Probability to be consistent with constant flux from VAR_CHI2_4
double
var_prob_5
Band 5 Probability to be consistent with constant flux from VAR_CHI2_5
double
x_ima
X image coordinate
pixel
double
x_ima_err
1-sigma error on X_IMA
pixel
double
y_ima
Y image coordinate
pixel
double
y_ima_err
1-sigma error on Y_IMA
double
catalogues.mv_xsa_epic_stack_cat_dr12_fdw
astcorr
Flag: observation was astrometrically corrected
boolean
bii
Galactic Latitude [degrees]
deg
double
cc_deofferr
double
cc_deoffset
double
cc_nmatches
int
cc_pofferr
double
cc_poffset
double
cc_raofferr
double
cc_raoffset
double
cc_refcat
char
cc_rot_corr
double
cc_rot_err
double
chi2prob_4xmmdr12
Probability of the DR7 source to be consistent with constant flux
double
dec_4xmmdr12
Mean declination (SC_)DEC of the nearest unique 4XMM-DR12 source
double
detid_4xmmdr12
long
dist_4xmmdr12
Distance to the nearest 4XMM-DR12 source / its detection in OBS_ID
double
dist_nn
The distance to the nearest neighbouring detection given in arcseconds.
double
dist_ref
Distance to the reference coordinates of the field
arcmin
double
ep_1_flux
EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_1_flux_err
Error on EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_2_flux
EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
ep_2_flux_err
Error on the EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
ep_3_flux
EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
ep_3_flux_err
Error on the EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
ep_4_flux
EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
ep_4_flux_err
Error on the EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
ep_5_flux
EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
ep_5_flux_err
Error on the EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
ep_cts
All EPIC number of counts
counts
double
ep_cts_err
1-sigma error on EP_CTS
counts
double
ep_det_ml
All-EPIC equivalent maximum detection likelihood
double
ep_flag
EPIC Quality Flag
char
ep_hr1
EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr1_err
Error on EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr2
EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr2_err
Error on EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr3
EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr3_err
Error on EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr4
EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
ep_hr4_err
Error on EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
epic_stack_cat_equatorial_spoint
Coordinates of the source on the celestial sphere given in RA and DEC (J2000).
char
epic_stack_cat_fov_scircle
Circle projected on the surface of the celestial sphere centered at the coordinates of the source given in RA and DEC (J2000) and a given radius of 15 arc min.
char
epic_stack_cat_galactic_spoint
Coordinates of the source on the celestial sphere given in latitude and longitude.
char
epic_xmm_stack_cat_oid
Internal identifier
int
ep_offax
double
ep_rate
All EPIC count rate
counts/s
double
ep_rate_err
1-sigma error on EP_RATE
counts/s
double
extent_ml
Likelihood of the detection being extended
double
fbr_var_chi2_21
Reduced chi square of EPIC band 2 to 1 inter-observation variability
double
fbr_var_chi2_31
Reduced chi square of EPIC band 3 to 1 inter-observation variability
double
fbr_var_chi2_32
Reduced chi square of EPIC band 3 to 2 inter-observation variability
double
fbr_var_chi2_41
Reduced chi square of EPIC band 4 to 1 inter-observation variability
double
fbr_var_chi2_42
Reduced chi square of EPIC band 4 to 2 inter-observation variability
double
fbr_var_chi2_43
Reduced chi square of EPIC band 4 to 3 inter-observation variability
double
fbr_var_chi2_51
Reduced chi square of EPIC band 5 to 1 inter-observation variability
double
fbr_var_chi2_52
Reduced chi square of EPIC band 5 to 2 inter-observation variability
double
fbr_var_chi2_53
Reduced chi square of EPIC band 5 to 3 inter-observation variability
double
fbr_var_chi2_54
Reduced chi square of EPIC band 5 to 4 inter-observation variability
double
fbr_var_dsig_21
Largest difference of EPIC band 2 to 1 flux ratios in terms of sigma
double
fbr_var_dsig_31
Largest difference of EPIC band 3 to 1 flux ratios in terms of sigma
double
fbr_var_dsig_32
Largest difference of EPIC band 3 to 2 flux ratios in terms of sigma
double
fbr_var_dsig_41
Largest difference of EPIC band 4 to 1 flux ratios in terms of sigma
double
fbr_var_dsig_42
Largest difference of EPIC band 4 to 2 flux ratios in terms of sigma
double
fbr_var_dsig_43
Largest difference of EPIC band 4 to 3 flux ratios in terms of sigma
double
fbr_var_dsig_51
Largest difference of EPIC band 5 to 1 flux ratios in terms of sigma
double
fbr_var_dsig_52
Largest difference of EPIC band 5 to 2 flux ratios in terms of sigma
double
fbr_var_dsig_53
Largest difference of EPIC band 5 to 3 flux ratios in terms of sigma
double
fbr_var_dsig_54
Largest difference of EPIC band 5 to 4 flux ratios in terms of sigma
double
fbr_var_prob_21
Probability that the flux band 2 to 1 variability is consistent
double
fbr_var_prob_31
Probability that the flux band 3 to 1 variability is consistent
double
fbr_var_prob_32
Probability that the flux band 3 to 2 variability is consistent
double
fbr_var_prob_41
Probability that the flux band 4 to 1 variability is consistent
double
fbr_var_prob_42
Probability that the flux band 4 to 2 variability is consistent
double
fbr_var_prob_43
Probability that the flux band 4 to 3 variability is consistent
double
fbr_var_prob_51
Probability that the flux band 5 to 1 variability is consistent
double
fbr_var_prob_52
Probability that the flux band 5 to 2 variability is consistent
double
fbr_var_prob_53
Probability that the flux band 5 to 3 variability is consistent
double
fbr_var_prob_54
Probability that the flux band 5 to 4 variability is consistent
double
fluxvar_1
Largest EPIC band 1 flux difference in terms of sigma
double
fluxvar_2
Largest EPIC band 2 flux difference in terms of sigma
double
fluxvar_3
Largest EPIC band 3 flux difference in terms of sigma
double
fluxvar_4
Largest EPIC band 4 flux difference in terms of sigma
double
fluxvar_5
Largest EPIC band 5 flux difference in terms of sigma
double
fratio
EPIC flux ratio
double
fratio_1
EPIC band 1 flux ration
double
fratio_1_err
1-sigma error on F_RATIO_1
double
fratio_2
EPIC band 2 flux ration
double
fratio_2_err
1-sigma error on F_RATIO_2
double
fratio_3
EPIC band 3 flux ration
double
fratio_3_err
1-sigma error on F_RATIO_3
double
fratio_4
EPIC band 4 flux ration
double
fratio_4_err
1-sigma error on F_RATIO_4
double
fratio_5
EPIC band 5 flux ration
double
fratio_5_err
1-sigma error on F_RATIO_5
double
fratio_err
1-sigma error on F_RATIO
double
fvar_4xmmdr12
Fractional intra-obs. excess variance of the nearest 4XMM-DR12 source
double
fvarerr_4xmmdr12
1-sigma error on FVAR_4XMM-DR12
double
lii
Galactic Longitude [degrees]
deg
double
m1_1_bg
M1 background map value in the 0.2-0.5 keV band
count/pixel
double
m1_1_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 1
double
m1_1_exp
PSF-weighted exposure of the detection in energy band 1 on EPIC/MOS1
s
double
m1_1_flux
EPIC/MOS1 Flux in Energy band 1
erg/cm²/s
double
m1_1_flux_err
1-sigma error on M1_2_FLUX
erg/cm²/s
double
m1_1_rate
M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_rate_err
Error on M1 count rate in the 0.2-0.5 keV band
counts/s
double
m1_1_vig
double
m1_2_bg
M1 background map value in the 0.5-1.0 keV band
count/pixel
double
m1_2_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 2
double
m1_2_exp
PSF-weighted exposure of the detection in energy band 2 on EPIC/MOS1
s
double
m1_2_flux
EPIC/MOS1 Flux in Energy band 2
erg/cm²/s
double
m1_2_flux_err
1-sigma error on M1_3_FLUX
erg/cm²/s
double
m1_2_rate
M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_2_rate_err
Error on M1 count rate in the 0.5-1.0 keV band
counts/s
double
m1_2_vig
double
m1_3_bg
M1 background map value in the 1.0-2.0 keV band
count/pixel
double
m1_3_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 3
double
m1_3_exp
PSF-weighted exposure of the detection in energy band 3 on EPIC/MOS1
s
double
m1_3_flux
EPIC/MOS1 Flux in Energy band 3
erg/cm²/s
double
m1_3_flux_err
1-sigma error on M1_4_FLUX
erg/cm²/s
double
m1_3_rate
M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_3_rate_err
Error on M1 count rate in the 1.0-2.0 keV band
counts/s
double
m1_3_vig
double
m1_4_bg
M1 background map value in the 2.0-4.5 keV band
count/pixel
double
m1_4_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 4
double
m1_4_exp
PSF-weighted exposure of the detection in energy band 4 on EPIC/MOS1
s
double
m1_4_flux
EPIC/MOS1 Flux in Energy band 3
erg/cm²/s
double
m1_4_flux_err
1-sigma error on M1_4_FLUX
erg/cm²/s
double
m1_4_rate
M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_4_rate_err
Error on M1 count rate in the 2.0-4.5 keV band
counts/s
double
m1_4_vig
double
m1_5_bg
M1 background map value in the 4.5-12.0 keV band
count/pixel
double
m1_5_det_ml
EPIC/MOS1 equ. maximum detection likelihood in energy band 5
double
m1_5_exp
PSF-weighted exposure of the detection in energy band 5 on EPIC/MOS1
s
double
m1_5_flux
EPIC/MOS1 Flux in Energy band 5
erg/cm²/s
double
m1_5_flux_err
1-sigma error on M1_5_FLUX
erg/cm²/s
double
m1_5_rate
M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_5_rate_err
Error on M1 count rate in the 4.5-12.0 keV band
counts/s
double
m1_5_vig
double
m1_bg
EPIC/MOS1 background map at detection position
counts/pixel
double
m1_bkg_cprob
double
m1_bkg_crarea
double
m1_cts
EPIC MOS1 number of counts
counts
double
m1_cts_err
1-sigma error on M1_CTS
counts
double
m1_det_ml
EPIC/MOS1 equ. maximum detection likelihood.
double
m1_exp
PSF-weighted exposure of the detection in EPIC/MOS1
s
double
m1_filter
char
m1_flag
MOS1 flag string made of the flags 1-12 (counted from left to right) for the MOS1 source detection.
char
m1_flux
Total EPIC/MOS1 flux
erg/cm²/s
double
m1_flux_err
1-sigma error on M1_1_FLUX
erg/cm²/s
double
m1_hr1
M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr1_err
Error on M1 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m1_hr2
M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr2_err
Error on M1 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m1_hr3
M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr3_err
Error on M1 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m1_hr4
M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_hr4_err
Error on M1 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m1_maskfrac
PSF-weighted detector coverage in EPIC/M1
double
m1_offax
double
m1_ontime
Total good exposure time in EPIC/MOS1
s
double
m1_pileup
Estimate of the pile-up level in EPIC/MOS1
double
m1_rate
Total EPIC/MOS1 count rate
counts/s
double
m1_rate_err
1-sigma error on M1_RATE
counts/s
double
m1_submode
char
m2_1_bg
M2 background map value in the 0.2-0.5 keV band
count/pixel
double
m2_1_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 1
double
m2_1_exp
PSF-weighted exposure of the detection in energy band 1 on EPIC/MOS2
s
double
m2_1_flux
EPIC/MOS2 Flux in Energy band 1
erg/cm²/s
double
m2_1_flux_err
1-sigma error on M2_1_FLUX
erg/cm²/s
double
m2_1_rate
M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_rate_err
Error on M2 count rate in the 0.2-0.5 keV band
counts/s
double
m2_1_vig
double
m2_2_bg
M2 background map value in the 0.5-1.0 keV band
count/pixel
double
m2_2_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 2
double
m2_2_exp
PSF-weighted exposure of the detection in energy band 2 on EPIC/MOS2
s
double
m2_2_flux
EPIC/MOS2 Flux in Energy band 2
erg/cm²/s
double
m2_2_flux_err
1-sigma error on M2_2_FLUX
erg/cm²/s
double
m2_2_rate
M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_2_rate_err
Error on M2 count rate in the 0.5-1.0 keV band
counts/s
double
m2_2_vig
double
m2_3_bg
M2 background map value in the 1.0-2.0 keV band
count/pixel
double
m2_3_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 3
double
m2_3_exp
PSF-weighted exposure of the detection in energy band 3 on EPIC/MOS2
s
double
m2_3_flux
EPIC/MOS2 Flux in Energy band 3
erg/cm²/s
double
m2_3_flux_err
1-sigma error on M2_3_FLUX
erg/cm²/s
double
m2_3_rate
M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_3_rate_err
Error on M2 count rate in the 1.0-2.0 keV band
counts/s
double
m2_3_vig
double
m2_4_bg
M2 background map value in the 2.0-4.5 keV band
count/pixel
double
m2_4_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 4
double
m2_4_exp
PSF-weighted exposure of the detection in energy band 4 on EPIC/MOS2
s
double
m2_4_flux
EPIC/MOS2 Flux in Energy band 4
erg/cm²/s
double
m2_4_flux_err
1-sigma error on M2_4_FLUX
erg/cm²/s
double
m2_4_rate
M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_4_rate_err
Error on M2 count rate in the 2.0-4.5 keV band
counts/s
double
m2_4_vig
double
m2_5_bg
M2 background map value in the 4.5-12.0 keV band
count/pixel
double
m2_5_det_ml
EPIC/MOS2 equ. maximum detection likelihood in energy band 5
double
m2_5_exp
PSF-weighted exposure of the detection in energy band 5 on EPIC/MOS2
s
double
m2_5_flux
EPIC/MOS2 Flux in Energy band 5
erg/cm²/s
double
m2_5_flux_err
1-sigma error on M2_5_FLUX
erg/cm²/s
double
m2_5_rate
M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_5_rate_err
Error on M2 count rate in the 4.5-12.0 keV band
counts/s
double
m2_5_vig
double
m2_bg
EPIC/MOS2 background map at detection position
counts/pixel
double
m2_bkg_cprob
double
m2_bkg_crarea
double
m2_cts
EPIC MOS2 number of counts
counts
double
m2_cts_err
1-sigma error on M2_CTS
counts
double
m2_det_ml
EPIC/MOS2 equ. maximum detection likelihood.
double
m2_exp
PSF-weighted exposure of the detection in EPIC/MOS1
s
double
m2_filter
char
m2_flag
MOS2 flag string made of the flags 1-12 (counted from left to right) for the MOS2 source detection.
char
m2_flux
Total EPIC/MOS2 flux
erg/cm²/s
double
m2_flux_err
1-sigma error on M2_FLUX
erg/cm²/s
double
m2_hr1
M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr1_err
Error on M2 hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
m2_hr2
M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr2_err
Error on M2 hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
m2_hr3
M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr3_err
Error on M2 hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
m2_hr4
M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_hr4_err
Error on M2 hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
m2_maskfrac
PSF-weighted detector coverage in EPIC/M2
double
m2_offax
double
m2_ontime
Total good exposure time in EPIC/MOS2
s
double
m2_pileup
Estimate of the pile-up level in EPIC/MOS2
double
m2_rate
EPIC/MOS2 count rate .
counts/s
double
m2_rate_err
1-sigma error on M2_RATE
counts/s
double
m2_submode
char
mjd_last
Modified Julian DATE JD-2400000.5 of the observation end
d
double
n_blend
Number of simultaneously fit sources
int
ndetect_4xmmdr12
Number of DR7 detections of the nearest unique 4XMM-DR12 source
int
n_exp
Number of instruments for which the source was fitted
int
n_exp_phot
Number of exposures used for PSF photometry
int
n_exp_sdet
Number of exposures used in source detection
int
npix
long
obs_class
int
obs_id
char
overlap
Flag: observation was astrometrically corrected
boolean
pa_pnt
double
pn_1_bg
PN background map value in the 0.2-0.5 keV band
count/pixel
double
pn_1_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 1
double
pn_1_exp
PSF-weighted exposure of the detection in energy band 1 on EPIC/PN
s
double
pn_1_flux
EPIC/PN flux on energy band 1
erg/cm²/s
double
pn_1_flux_err
1-sigma error on PN_FLUX_1
erg/cm²/s
double
pn_1_rate
PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_rate_err
Error on the PN count rate in the 0.2-0.5 keV band
count/s
double
pn_1_vig
double
pn_2_bg
PN background map value in the 0.5-1.0 keV band
count/pixel
double
pn_2_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 2
double
pn_2_exp
PSF-weighted exposure of the detection in energy band 2 on EPIC/PN
s
double
pn_2_flux
EPIC/PN flux on energy band 2
erg/cm²/s
double
pn_2_flux_err
1-sigma error on PN_FLUX_2
erg/cm²/s
double
pn_2_rate
PN count rate in the 0.5-1.0 keV band
count/s
double
pn_2_rate_err
Error on PN count rate in the 0.5-1.0 keV band
counts/s
double
pn_2_vig
double
pn_3_bg
PN background map value in the 1.0-2.0 keV band
count/pixel
double
pn_3_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 3
double
pn_3_exp
PSF-weighted exposure of the detection in energy band 3 on EPIC/PN
s
double
pn_3_flux
EPIC/PN flux on energy band 3
erg/cm²/s
double
pn_3_flux_err
1-sigma error on PN_FLUX_3
erg/cm²/s
double
pn_3_rate
PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_3_rate_err
Error on PN count rate in the 1.0-2.0 keV band
counts/s
double
pn_3_vig
double
pn_4_bg
PN background map value in the 2.0-4.5 keV band
count/pixel
double
pn_4_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 4
double
pn_4_exp
PSF-weighted exposure of the detection in energy band 4 on EPIC/PN
s
double
pn_4_flux
EPIC/PN flux on energy band 4
erg/cm²/s
double
pn_4_flux_err
1-sigma error on PN_FLUX_4
erg/cm²/s
double
pn_4_rate
PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_4_rate_err
Error on PN count rate in the 2.0-4.5 keV band
counts/s
double
pn_4_vig
double
pn_5_bg
PN background map value in the 4.5-12.0 keV band
count/pixel
double
pn_5_det_ml
EPIC/PN equ. maximum detection likelihood in energy band 5.
double
pn_5_exp
PSF-weighted exposure of the detection in energy band 5 on EPIC/PN
s
double
pn_5_flux
EPIC/PN Flux in Energy band 5
erg/cm²/s
double
pn_5_flux_err
1-sigma error on PN_5_FLUX
erg/cm²/s
double
pn_5_rate
PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_5_rate_err
Error on PN count rate in the 4.5-12.0 keV band
counts/s
double
pn_5_vig
double
pn_bg
EPIC/PN background map at detection position
counts/pixel
double
pn_bkg_cprob
double
pn_bkg_crarea
double
pn_cts
EPIC PN number of counts
counts
double
pn_cts_err
1-sigma error on PN_CTS
counts
double
pn_det_ml
EPIC/PN equ. maximum detection likelihood
double
pn_exp
PSF-weighted exposure of the detection in EPIC/PN
s
double
pn_filter
char
pn_flag
PN flag string made of the flags 1-12 (counted from left to right) for the PN source detection.
char
pn_flux
Total EPIC/pn flux
erg/cm²/s
double
pn_flux_err
1-sigma error on PN_FLUX
erg/cm²/s
double
pn_hr1
PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr1_err
Error on PN hardness ratio between the 0.2-0.5 keV and 0.5-1.0 keV bands
double
pn_hr2
PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr2_err
Error on PN hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
pn_hr3
PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr3_err
Error on PN hardness ratio between the 1.0-2.0 keV and 2.0-4.5 keV bands
double
pn_hr4
PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_hr4_err
Error on PN hardness ratio between the 2.0-4.5 keV and 4.5-12.0 keV bands
double
pn_maskfrac
PSF-weighted detector coverage in EPIC/PN
double
pn_offax
double
pn_ontime
Total good exposure time all-EPIC
s
double
pn_pileup
Estimate of the pile-up level in EPIC/pn
double
pn_rate
Total EPIC/pn count rate
counts/s
double
pn_rate_err
1-sigma error on PN_RATE
counts/s
double
pn_submode
char
poserr_4xmmdr12
Statistical & systematic position error of the 4XMM-DR12 source
double
ra_4xmmdr12
Mean right ascension (SC_)RA of the nearest unique 4XMM-DR12 source
double
radec_err
Radial error on the position, computed as sqrt(ra_err2 + dec_err2), in arcsecs, where ra_err and dec_err are the 1 sigma uncertainties in the RA and DEC coordinates respectively.
double
revolut
int
srcid
A unique number assigned to a group of catalogue entries which are assumed to be the same source.
long
srcid_4xmmdr12
Source identifier of the nearest unique source in 4XMM-DR12
long
stack_flag
Integer representation of the stack detection flags
int
sum_flag_4xmmdr12
Summary quality flag of the nearest unique 4XMM-DR12 source
int
sum_flag_min_4xmmdr12
Best quality flag of the detections of the nearest 4XMM-DR12 source
int
url_4xmmdr12
Webpage URL of the nearest 4XMM-DR12 source
char
var_chi2
Reduced chi-square of EPIC inter-observation variability.
double
var_chi2_1
Reduced chi-square of EPIC band 1 inter-observation variability.
double
var_chi2_2
Reduced chi-square of EPIC band 2 inter-observation variability.
double
var_chi2_3
Reduced chi-square of EPIC band 3 inter-observation variability.
double
var_chi2_4
Reduced chi-square of EPIC band 4 inter-observation variability.
double
var_chi2_5
Reduced chi-square of EPIC band 5 inter-observation variability.
double
var_flag_4xmmdr12
Intra-observation variability flag of the nearest 4XMM-DR12 source
boolean
var_prob
Probability to be consistent with constant flux from VAR_CHI2
double
var_prob_1
Band 1 Probability to be consistent with constant flux from VAR_CHI2_1
double
var_prob_2
Band 2 Probability to be consistent with constant flux from VAR_CHI2_2
double
var_prob_3
Band 3 Probability to be consistent with constant flux from VAR_CHI2_3
double
var_prob_4
Band 4 Probability to be consistent with constant flux from VAR_CHI2_4
double
var_prob_5
Band 5 Probability to be consistent with constant flux from VAR_CHI2_5
double
x_ima
X image coordinate
pixel
double
x_ima_err
1-sigma error on X_IMA
pixel
double
y_ima
Y image coordinate
pixel
double
y_ima_err
1-sigma error on Y_IMA
double
iauname
IAU name of the source
char
primary
iauname_4xmmdr12
IAU name assigned to the nearest unique 4XMM-DR12 source
char
primary
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
primary
ep_flux
EPIC flux in the 0.2-12.0 keV band
erg/cm²/s
double
primary
ep_flux_err
1-sigma Error on EPIC flux in the 0.2-12.0 keV band
erg/cm²/s
double
primary
n_contrib
Number of pointings in which the source was fitted
pixel
int
primary
n_obs
Number of observations involved in the stack
int
primary
mjd_first
Modified Julian DATE JD-2400000.5 of the observation start
d
double
primary
ep_ontime
The EPIC ontime value, given in seconds, is the total good exposure time (after GTI filtering)
s
double
primary
extent
Extent radius
arcsec
double
primary
extent_err
1-sigma error on EXTENT
arcsec
double
primary
fluxvar
Largest EPIC flux difference in terms of sigma
double
primary
catalogues.mv_xsa_epic_stack_cat_fdw
The XMM-Newton Serendipitous Source Catalogues from stacked XMM-Newton observations: 4XMM-DR14s
astcorr
Flag: observation was astrometrically corrected
char
cc_deofferr
1-sigma error on CC_DEOFFSET
arcsec
double
cc_deoffset
The field shift in DEC as derived by the SAS task catcorr
arcsec
double
cc_nmatches
catcorr number of usable matches with the reference catalogue
int
cc_pofferr
1-sigma error on CC_POFFSET
arcsec
double
cc_poffset
The absolute offset between the original and the corrected source position as derived by the SAS task catcorr
arcsec
double
cc_raofferr
1-sigma error on CC_RAOFFSET
arcsec
double
cc_raoffset
The field shift in RA as derived by the SAS task catcorr
arcsec
double
cc_refcat
catcorr reference catalogue
char
cc_rot_corr
The field rotation as derived by the SAS task catcorr
degree
double
cc_rot_err
1-sigma error on CC_ROT_CORR
degree
double
chi2prob_detcat
Probability of the DR7 source to be consistent with constant flux
double
dec_detcat
Mean declination (SC_)DEC of the nearest unique 4XMM-DR14 source
double
detid_detcat
Detection identifier of the unique 4XMM-DR14 source in OBS_ID
long
dist_detcat
Distance to the nearest 4XMM-DR14 source / its detection in OBS_ID
double
dist_nn
The distance to the nearest neighbouring detection given in arcseconds.
double
dist_ref
Distance to the reference coordinates of the field
arcmin
double
ep_1_flux
EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_1_flux_err
Error on EPIC flux in the 0.2-0.5 keV band
erg/cm**2/s
double
ep_2_flux
EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
ep_2_flux_err
Error on the EPIC flux in the 0.5-1.0 keV band
erg/cm**2/s
double
ep_3_flux
EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
ep_3_flux_err
Error on the EPIC flux in the 1.0-2.0 keV band
erg/cm**2/s
double
ep_4_flux
EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
ep_4_flux_err
Error on the EPIC flux in the 2.0-4.5 keV band
erg/cm**2/s
double
ep_5_flux
EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
ep_5_flux_err
Error on the EPIC flux in the 4.5-12.0 keV band
erg/cm**2/s
double
ep_cts
All EPIC number of counts
counts
double
ep_cts_err
1-sigma error on EP_CTS
counts
double
ep_det_ml
All-EPIC equivalent maximum detection likelihood
double
ep_flag
EPIC Quality Flag
char
ep_hr1
EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr1_err
Error on EPIC Hardness Ratio 1, between counts in the 0.5-1.0 and the 0.2-0.5 keV energy bands
double
ep_hr2
EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr2_err
Error on EPIC hardness ratio between the 0.5-1.0 keV and 1.0-2.0 keV bands
double
ep_hr3
EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr3_err
Error on EPIC Hardness Ratio 3, between the counts in the 2.0-4.5 and 1.0-2.0 keV energy bands
double
ep_hr4
EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
ep_hr4_err
Error on EPIC Hardness Ratio 4, between the counts in the 4.5-12.0 and 2.0-4.5 keV energy bands
double
epic_stack_cat_equatorial_spoint
Coordinates of the source on the celestial sphere given in RA and DEC (J2000).
char
epic_stack_cat_fov_scircle
Circle projected on the surface of the celestial sphere centered at the coordinates of the source given in RA and DEC (J2000) and a given radius of 15 arc min.
char
epic_stack_cat_galactic_spoint
Coordinates of the source on the celestial sphere given in latitude and longitude.
char
epic_xmm_stack_cat_oid
Internal identifier
int
ep_rate
All EPIC count rate
counts/s
double
ep_rate_err
1-sigma error on EP_RATE
counts/s
double
extent_ml
Likelihood of the detection being extended
double
fbr_var_chi2_21
Reduced chi square of EPIC band 2 to 1 inter-observation variability
char
fbr_var_chi2_31
Reduced chi square of EPIC band 3 to 1 inter-observation variability
char
fbr_var_chi2_32
Reduced chi square of EPIC band 3 to 2 inter-observation variability
char
fbr_var_chi2_41
Reduced chi square of EPIC band 4 to 1 inter-observation variability
char
fbr_var_chi2_42
Reduced chi square of EPIC band 4 to 2 inter-observation variability
char
fbr_var_chi2_43
Reduced chi square of EPIC band 4 to 3 inter-observation variability
char
fbr_var_chi2_51
Reduced chi square of EPIC band 5 to 1 inter-observation variability
char
fbr_var_chi2_52
Reduced chi square of EPIC band 5 to 2 inter-observation variability
char
fbr_var_chi2_53
Reduced chi square of EPIC band 5 to 3 inter-observation variability
char
fbr_var_chi2_54
Reduced chi square of EPIC band 5 to 4 inter-observation variability
char
fbr_var_dsig_21
Largest difference of EPIC band 2 to 1 flux ratios in terms of sigma
char
fbr_var_dsig_31
Largest difference of EPIC band 3 to 1 flux ratios in terms of sigma
char
fbr_var_dsig_32
Largest difference of EPIC band 3 to 2 flux ratios in terms of sigma
char
fbr_var_dsig_41
Largest difference of EPIC band 4 to 1 flux ratios in terms of sigma
char
fbr_var_dsig_42
Largest difference of EPIC band 4 to 2 flux ratios in terms of sigma
char
fbr_var_dsig_43
Largest difference of EPIC band 4 to 3 flux ratios in terms of sigma
char
fbr_var_dsig_51
Largest difference of EPIC band 5 to 1 flux ratios in terms of sigma
char
fbr_var_dsig_52
Largest difference of EPIC band 5 to 2 flux ratios in terms of sigma
char
fbr_var_dsig_53
Largest difference of EPIC band 5 to 3 flux ratios in terms of sigma
char
fbr_var_dsig_54
Largest difference of EPIC band 5 to 4 flux ratios in terms of sigma
char
fbr_var_prob_21
Probability that the flux band 2 to 1 variability is consistent
double
fbr_var_prob_31
Probability that the flux band 3 to 1 variability is consistent
double
fbr_var_prob_32
Probability that the flux band 3 to 2 variability is consistent
double
fbr_var_prob_41
Probability that the flux band 4 to 1 variability is consistent
double
fbr_var_prob_42
Probability that the flux band 4 to 2 variability is consistent
double
fbr_var_prob_43
Probability that the flux band 4 to 3 variability is consistent
double
fbr_var_prob_51
Probability that the flux band 5 to 1 variability is consistent
double
fbr_var_prob_52
Probability that the flux band 5 to 2 variability is consistent
double
fbr_var_prob_53
Probability that the flux band 5 to 3 variability is consistent
double
fbr_var_prob_54
Probability that the flux band 5 to 4 variability is consistent
double
fc_icon_location
char
fc_icon_preview_location
char
fc_postcard_location
char
fratio
EPIC flux ratio
double
fratio_err
1-sigma error on F_RATIO
double
fvar_detcat
Fractional intra-obs. excess variance of the nearest 4XMM-DR14 source
double
fvarerr_detcat
1-sigma error on FVAR_4XMM-DR14
double
lc_icon_location
char
lc_icon_preview_location
char
lc_postcard_location
char
m1_bkg_cprob
EPIC/MOS1 Cauchy probability derived from M1_BKG_CRAREA
double
m1_bkg_crarea
EPIC/mos1 background rate per area
counts.s-1.arcsec-2
double
m1_maskfrac
PSF-weighted detector coverage in EPIC/M1
double
m1_ontime
Total good exposure time in EPIC/MOS1
s
double
m1_pileup
Estimate of the pile-up level in EPIC/MOS1
char
m2_bkg_cprob
EPIC/MOS2 Cauchy probability derived from M2_BKG_CRAREA
double
m2_bkg_crarea
EPIC/mos2 background rate per area
counts.s-1.arcsec-2
double
m2_maskfrac
PSF-weighted detector coverage in EPIC/M2
double
m2_ontime
Total good exposure time in EPIC/MOS2
s
double
m2_pileup
Estimate of the pile-up level in EPIC/MOS2
char
mjd_last
Modified Julian DATE JD-2400000.5 of the observation end
d
double
n_blend
Number of simultaneously fit sources
int
ndetect_detcat
Number of DR7 detections of the nearest unique 4XMM-DR14 source
int
n_exp
Number of instruments for which the source was fitted
int
npix
int
obs_id
XMM-Newton observation identification
char
overlap
Flag: observation was astrometrically corrected
char
pa_pnt
Mean position angle of the spacecraft
deg
double
pn_1_bg
PN background map value in the 0.2-0.5 keV band
count/pixel
double
pn_1_exp
PSF-weighted exposure of the detection in energy band 1 on EPIC/PN
s
double
pn_1_vig
EPIC/pn vignetting factor in energy band 1 in this observation
double
pn_2_bg
PN background map value in the 0.5-1.0 keV band
count/pixel
double
pn_2_exp
PSF-weighted exposure of the detection in energy band 2 on EPIC/PN
s
double
pn_2_vig
EPIC/pn vignetting factor in energy band 2 in this observation
double
pn_3_bg
PN background map value in the 1.0-2.0 keV band
count/pixel
double
pn_3_exp
PSF-weighted exposure of the detection in energy band 3 on EPIC/PN
s
double
pn_3_vig
EPIC/pn vignetting factor in energy band 3 in this observation
double
pn_4_bg
PN background map value in the 2.0-4.5 keV band
count/pixel
double
pn_4_exp
PSF-weighted exposure of the detection in energy band 4 on EPIC/PN
s
double
pn_4_vig
EPIC/pn vignetting factor in energy band 4 in this observation
double
pn_5_bg
PN background map value in the 4.5-12.0 keV band
count/pixel
double
pn_5_exp
PSF-weighted exposure of the detection in energy band 5 on EPIC/PN
s
double
pn_5_vig
EPIC/pn vignetting factor in energy band 5 in this observation
double
pn_bg
EPIC/PN background map at detection position
counts/pixel
double
pn_bkg_cprob
EPIC/pn Cauchy probability derived from PN_BKG_CRAREA
double
pn_bkg_crarea
EPIC/pn background rate per area
counts.s-1.arcsec-2
double
pn_cts
EPIC PN number of counts
counts
double
pn_cts_err
1-sigma error on PN_CTS
counts
double
pn_exp
PSF-weighted exposure of the detection in EPIC/PN
s
double
pn_flag
PN flag string made of the flags 1-12 (counted from left to right) for the PN source detection.
char
pn_flux
Total EPIC/pn flux
erg/cm²/s
double
pn_flux_err
1-sigma error on PN_FLUX
erg/cm²/s
double
pn_maskfrac
PSF-weighted detector coverage in EPIC/PN
double
pn_ontime
Total good exposure time all-EPIC
s
double
pn_pileup
Estimate of the pile-up level in EPIC/pn
char
pn_rate
Total EPIC/pn count rate
counts/s
double
pn_rate_err
1-sigma error on PN_RATE
counts/s
double
poserr_detcat
Statistical & systematic position error of the 4XMM-DR14 source
double
radec_err
Radial error on the position, computed as sqrt(ra_err2 + dec_err2), in arcsecs, where ra_err and dec_err are the 1 sigma uncertainties in the RA and DEC coordinates respectively.
double
ra_detcat
Mean right ascension (SC_)RA of the nearest unique 4XMM-DR14 source
double
revolut
XMM-Newton revolution number of the observation
orbit
int
srcid
A unique number assigned to a group of catalogue entries which are assumed to be the same source.
long
srcid_detcat
Source identifier of the nearest unique source in 4XMM-DR14
long
stack_flag
Integer representation of the stack detection flags
int
sum_flag_detcat
Summary quality flag of the nearest unique 4XMM-DR14 source
int
var_chi2
Reduced chi-square of EPIC inter-observation variability.
double
var_chi2_1
Reduced chi-square of EPIC band 1 inter-observation variability.
double
var_chi2_2
Reduced chi-square of EPIC band 2 inter-observation variability.
double
var_chi2_3
Reduced chi-square of EPIC band 3 inter-observation variability.
double
var_chi2_4
Reduced chi-square of EPIC band 4 inter-observation variability.
double
var_chi2_5
Reduced chi-square of EPIC band 5 inter-observation variability.
double
var_flag_detcat
Intra-observation variability flag of the nearest 4XMM-DR14 source
char
iauname
IAU name of the source
meta.id;meta.main
char
primary
iauname_detcat
IAU name assigned to the nearest unique 4XMM-DR14 source
char
primary
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
primary
ep_flux
EPIC flux in the 0.2-12.0 keV band
erg/cm²/s
double
primary
ep_flux_err
1-sigma Error on EPIC flux in the 0.2-12.0 keV band
erg/cm²/s
double
primary
n_contrib
Number of pointings in which the source was fitted
pixel
int
primary
n_obs
Number of observations involved in the stack
int
primary
mjd_first
Modified Julian DATE JD-2400000.5 of the observation start
d
double
primary
ep_ontime
The EPIC ontime value, given in seconds, is the total good exposure time (after GTI filtering)
s
double
primary
extent
Extent radius
arcsec
double
primary
extent_err
1-sigma error on EXTENT
arcsec
double
primary
fluxvar
Largest EPIC flux difference in terms of sigma
double
primary
catalogues.mv_xsa_om_source_cat_5_fdw
b_ab_flux_err
B Filter Flux Err
erg s-1 cm-2 A-1
double
b_ab_mag
B AB_Magnitude
double
b_ab_mag_err
B AB_Magnitude Err
double
b_extended_flag
B Filter Extended Flag
int
bii
Galactic Latitude [degrees]
deg
double
b_major_axis
float
b_minor_axis
float
b_posang
float
b_quality_flag
B Filter Quality Flag
int
b_quality_flag_str
B Quality Flag Str
char
b_rate
float
b_rate_err
float
b_signif
B Detection Significance
double
b_sky_image
B Filter Mosaic/Stacked image
char
b_srcdist
float
b_vega_mag
B Vega Mag
double
b_vega_mag_err
B Vega Mag Err
double
date_end
OM observation end time in UTC
char
date_obs
OM observation start time in UTC
char
dec_dms
Declination (J2000) [dd:mm:ss.sss]
char
duration
Exposure on time
int
lii
Galactic Longitude [degrees]
deg
double
n_obsid
int
npix
Healpix pixel of the center for nside 256
long
n_summary
int
om_source_cat_equatorial_spoint
char
om_source_cat_fov_scircle
char
om_source_cat_galactic_spoint
char
om_source_cat_oid
int
ra_hms
Right Ascension (J2000) [hh:mm:ss.sss]
char
srcnum
Source number
int
u_ab_flux_err
U Filter Flux Err
erg s-1 cm-2 A-1
double
u_ab_mag
U AB_Magnitude
double
u_ab_mag_err
U AB_Magnitude Err
double
u_extended_flag
U Filter Extended Flag
int
u_major_axis
float
u_minor_axis
float
u_posang
float
u_quality_flag
U Filter Quality Flag
int
u_quality_flag_str
U Quality Flag Str
char
u_rate
float
u_rate_err
float
u_signif
U Detection Significance
double
u_sky_image
U Filter Mosaic/Stacked image
char
u_srcdist
float
u_vega_mag
U Vega Mag
double
u_vega_mag_err
U Vega Mag Err
double
uvm2_ab_flux_err
UVM2 Filter Flux Err
erg s-1 cm-2 A-1
double
uvm2_ab_mag
UVM2 AB_Magnitude
double
uvm2_ab_mag_err
UVM2 AB_Magnitude Err
double
uvm2_extended_flag
UVM2 Filter Extended Flag
int
uvm2_major_axis
float
uvm2_minor_axis
float
uvm2_posang
float
uvm2_quality_flag
UVM2 Filter Quality Flag
int
uvm2_quality_flag_str
UVM2 Quality Flag Str
char
uvm2_rate
float
uvm2_rate_err
float
uvm2_signif
UVM2 Detection Significance
double
uvm2_sky_image
UVM2 Filter Mosaic/Stacked image
char
uvm2_srcdist
float
uvm2_vega_mag
UVM2 Vega Mag
double
uvm2_vega_mag_err
UVM2 Vega Mag Err
double
uvw1_ab_flux_err
UVW1 Filter Flux Err
erg s-1 cm-2 A-1
double
uvw1_ab_mag
UVW1 AB_Magnitude
double
uvw1_ab_mag_err
UVW1 AB_Magnitude Err
double
uvw1_extended_flag
UVW1 Filter Extended Flag
int
uvw1_major_axis
float
uvw1_minor_axis
float
uvw1_posang
float
uvw1_quality_flag
UVW1 Filter Quality Flag
int
uvw1_quality_flag_str
UVW1 Quality Flag Str
char
uvw1_rate
float
uvw1_rate_err
float
uvw1_signif
UVW1 Detection Significance
double
uvw1_sky_image
UVW1 Filter Mosaic/Stacked image
char
uvw1_srcdist
float
uvw1_vega_mag
UVW1 Vega Mag
double
uvw1_vega_mag_err
UVW1 Vega Mag Err
double
uvw2_ab_flux_err
UVW2 Filter Flux Err
erg s-1 cm-2 A-1
double
uvw2_ab_mag
UVW2 AB_Magnitude
double
uvw2_ab_mag_err
UVW2 AB_Magnitude Err
double
uvw2_extended_flag
UVW2 Filter Extended Flag
int
uvw2_major_axis
float
uvw2_minor_axis
float
uvw2_posang
float
uvw2_quality_flag
UVW2 Filter Quality Flag
int
uvw2_quality_flag_str
UVW2 Quality Flag Str
char
uvw2_rate
float
uvw2_rate_err
float
uvw2_signif
UVW2 Detection Significance
double
uvw2_sky_image
UVW2 Filter Mosaic/Stacked image
char
uvw2_srcdist
float
uvw2_vega_mag
UVW2 Vega Mag
double
uvw2_vega_mag_err
UVW2 Vega Mag Err
double
v_ab_flux_err
V Filter Flux Err
erg s-1 cm-2 A-1
double
v_ab_mag
V AB_Magnitude
double
v_ab_mag_err
V AB_Magnitude Err
double
v_extended_flag
V Filter Extended Flag
int
v_major_axis
float
v_minor_axis
float
v_posang
float
v_quality_flag
V Filter Quality Flag
int
v_quality_flag_str
V Quality Flag Str
char
v_rate
float
v_rate_err
float
v_signif
V Detection Significance
double
v_sky_image
V Filter Mosaic/Stacked image
char
v_srcdist
float
v_vega_mag
V Vega Mag
double
v_vega_mag_err
V Vega Mag Err
double
iauname
The IAU name assigned to the unique SRCID
meta.id;meta.main
char
primary
observation_id
The XMM-Newton observation identification.
char
primary
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
primary
poserr
Position Error
arcsec
double
primary
uvw1_ab_flux
UVW1 Filter Flux
erg s-1 cm-2 A-1
double
primary
uvw2_ab_flux
UVW2 Filter Flux
erg s-1 cm-2 A-1
double
primary
uvm2_ab_flux
UVM2 Filter Flux
erg s-1 cm-2 A-1
double
primary
u_ab_flux
U Filter Flux
erg s-1 cm-2 A-1
double
primary
v_ab_flux
V Filter Flux
erg s-1 cm-2 A-1
double
primary
b_ab_flux
B Filter Flux
erg s-1 cm-2 A-1
double
primary
catalogues.mv_xsa_om_source_cat_6_fdw
b_ab_flux_err
B Filter Flux Err
erg s-1 cm-2 A-1
double
b_ab_mag
B AB_Magnitude
double
b_ab_mag_err
B AB_Magnitude Err
double
b_extended_flag
B Filter Extended Flag
int
bii
Galactic Latitude [degrees]
deg
double
b_major_axis
float
b_minor_axis
float
b_posang
float
b_quality_flag
B Filter Quality Flag
int
b_quality_flag_st
B Quality Flag Str
char
b_rate
float
b_rate_err
float
b_signif
B Detection Significance
double
b_sky_image
B Filter Mosaic/Stacked image
char
b_srcdist
float
b_vega_mag
B Vega Mag
double
b_vega_mag_err
B Vega Mag Err
double
date_end
OM observation end time in UTC
char
date_obs
OM observation start time in UTC
char
dec_dms
Declination (J2000) [dd:mm:ss.sss]
char
duration
Exposure on time
int
lii
Galactic Longitude [degrees]
deg
double
n_obsid
int
npix
Healpix pixel of the center for nside 256
long
n_summary
int
om_source_cat_equatorial_spoint
char
om_source_cat_fov_scircle
char
om_source_cat_galactic_spoint
char
om_source_cat_oid
int
ra_hms
Right Ascension (J2000) [hh:mm:ss.sss]
char
srcnum
Source number
int
u_ab_flux_err
U Filter Flux Err
erg s-1 cm-2 A-1
double
u_ab_mag
U AB_Magnitude
double
u_ab_mag_err
U AB_Magnitude Err
double
u_extended_flag
U Filter Extended Flag
int
u_major_axis
float
u_minor_axis
float
u_posang
float
u_quality_flag
U Filter Quality Flag
int
u_quality_flag_st
U Quality Flag Str
char
u_rate
float
u_rate_err
float
u_signif
U Detection Significance
double
u_sky_image
U Filter Mosaic/Stacked image
char
u_srcdist
float
u_vega_mag
U Vega Mag
double
u_vega_mag_err
U Vega Mag Err
double
uvm2_ab_flux_err
UVM2 Filter Flux Err
erg s-1 cm-2 A-1
double
uvm2_ab_mag
UVM2 AB_Magnitude
double
uvm2_ab_mag_err
UVM2 AB_Magnitude Err
double
uvm2_extended_flag
UVM2 Filter Extended Flag
int
uvm2_major_axis
float
uvm2_minor_axis
float
uvm2_posang
float
uvm2_quality_flag
UVM2 Filter Quality Flag
int
uvm2_quality_flag_st
UVM2 Quality Flag Str
char
uvm2_rate
float
uvm2_rate_err
float
uvm2_signif
UVM2 Detection Significance
double
uvm2_sky_image
UVM2 Filter Mosaic/Stacked image
char
uvm2_srcdist
float
uvm2_vega_mag
UVM2 Vega Mag
double
uvm2_vega_mag_err
UVM2 Vega Mag Err
double
uvw1_ab_flux_err
UVW1 Filter Flux Err
erg s-1 cm-2 A-1
double
uvw1_ab_mag
UVW1 AB_Magnitude
double
uvw1_ab_mag_err
UVW1 AB_Magnitude Err
double
uvw1_extended_flag
UVW1 Filter Extended Flag
int
uvw1_major_axis
float
uvw1_minor_axis
float
uvw1_posang
float
uvw1_quality_flag
UVW1 Filter Quality Flag
int
uvw1_quality_flag_st
UVW1 Quality Flag Str
char
uvw1_rate
float
uvw1_rate_err
float
uvw1_signif
UVW1 Detection Significance
double
uvw1_sky_image
UVW1 Filter Mosaic/Stacked image
char
uvw1_srcdist
float
uvw1_vega_mag
UVW1 Vega Mag
double
uvw1_vega_mag_err
UVW1 Vega Mag Err
double
uvw2_ab_flux_err
UVW2 Filter Flux Err
erg s-1 cm-2 A-1
double
uvw2_ab_mag
UVW2 AB_Magnitude
double
uvw2_ab_mag_err
UVW2 AB_Magnitude Err
double
uvw2_extended_flag
UVW2 Filter Extended Flag
int
uvw2_major_axis
float
uvw2_minor_axis
float
uvw2_posang
float
uvw2_quality_flag
UVW2 Filter Quality Flag
int
uvw2_quality_flag_st
UVW2 Quality Flag Str
char
uvw2_rate
float
uvw2_rate_err
float
uvw2_signif
UVW2 Detection Significance
double
uvw2_sky_image
UVW2 Filter Mosaic/Stacked image
char
uvw2_srcdist
float
uvw2_vega_mag
UVW2 Vega Mag
double
uvw2_vega_mag_err
UVW2 Vega Mag Err
double
v_ab_flux_err
V Filter Flux Err
erg s-1 cm-2 A-1
double
v_ab_mag
V AB_Magnitude
double
v_ab_mag_err
V AB_Magnitude Err
double
v_extended_flag
V Filter Extended Flag
int
v_major_axis
float
v_minor_axis
float
v_posang
float
v_quality_flag
V Filter Quality Flag
int
v_quality_flag_st
V Quality Flag Str
char
v_rate
float
v_rate_err
float
v_signif
V Detection Significance
double
v_sky_image
V Filter Mosaic/Stacked image
char
v_srcdist
float
v_vega_mag
V Vega Mag
double
v_vega_mag_err
V Vega Mag Err
double
iauname
The IAU name assigned to the unique SRCID
meta.id;meta.main
char
primary
obsid
The XMM-Newton observation identification.
char
primary
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
primary
poserr
Position Error
arcsec
double
primary
uvw1_ab_flux
UVW1 Filter Flux
erg s-1 cm-2 A-1
double
primary
uvw2_ab_flux
UVW2 Filter Flux
erg s-1 cm-2 A-1
double
primary
uvm2_ab_flux
UVM2 Filter Flux
erg s-1 cm-2 A-1
double
primary
u_ab_flux
U Filter Flux
erg s-1 cm-2 A-1
double
primary
v_ab_flux
V Filter Flux
erg s-1 cm-2 A-1
double
primary
b_ab_flux
B Filter Flux
erg s-1 cm-2 A-1
double
primary
catalogues.mv_xsa_om_source_cat_fdw
The XMM-Newton Serendipitous Ultraviolet Source Survey (XMM-SUSS) is a catalog of ultraviolet (UV) sources detected serendipitously by the Optical Monitor (XMM-OM) on board the XMM-Newton observatory. The current version is SUSS-6.2.
b_ab_flux_err
Source flux error for the filter B
erg/s/cm**2/A
double
b_ab_mag
Source AB magnitude for the filter B
mag
double
b_ab_mag_err
Source AB magnitude error, filter B
mag
double
b_extended_flag
Source extended flag for the filter B
int
bii
Source galactic latitude
degrees
double
b_major_axis
Source major semi-axis for the filter B
arcsec
double
b_minor_axis
Source minor semi-axis for the filter B
arcsec
double
b_posang
Source position angle for the filter B
degree
double
b_quality_flag
Source quality flag for the filter B
int
b_quality_flag_st
Source quality flag string, filter B
char
b_rate
Source count rate for the filter B
count/sec
double
b_rate_err
Source count rate error, filter B
count/sec
double
b_signif
Source significance for the filter B
sigma
double
b_sky_image
Source detected in stacked images filter B
char
b_srcdist
Dist. to the nearest source, B filter
arcsec
double
b_vega_mag
Source Vega magnitude for the filter B
mag
double
b_vega_mag_err
Source Vega magnitude error, filter B
mag
double
date_end
OM observation end time in UTC
char
date_obs
OM observation start time in UTC
char
dec_dms
Source Declination coordinate in DMS
char
duration
Exposure on time
int
fast_id
Fast timeseries source identification
char
primary
lii
Source galactic longtude
degrees
double
n_obsid
Number of observation IDs for this source
int
npix
long
n_summary
Index in the SUMMARY table for the source OBSID
long
obsid
Source OBSID number
meta.id;meta.main
char
primary
om_source_cat_equatorial_spoint
Coordinates of the source on the celestial sphere given in RA and DEC (J2000).
char
om_source_cat_fov_scircle
Circle projected on the surface of the celestial sphere centered at the coordinates of the source given in RA and DEC (J2000) and a given radius of 15 arc min.
char
om_source_cat_galactic_spoint
Coordinates of the source on the celestial sphere given in latitude and longitude.
char
om_source_cat_oid
int
ra_hms
Source Right Ascension in hour units
char
src_id
Source number in observation
int
srcnum
Source number in this catalogue
long
u_ab_flux_err
Source flux error for the filter U
erg/s/cm**2/A
double
u_ab_mag
Source AB magnitude for the filter U
mag
double
u_ab_mag_err
Source AB magnitude error, filter U
mag
double
u_extended_flag
Source extended flag for the filter U
int
u_major_axis
Source major semi-axis for the filter U
arcsec
double
u_minor_axis
Source minor semi-axis for the filter U
arcsec
double
u_posang
Source position angle for the filter U
degree
double
u_quality_flag
Source quality flag for the filter U
int
u_quality_flag_st
Source quality flag string, filter U
char
u_rate
Source count rate for the filter U
count/sec
double
u_rate_err
Source count rate error, filter U
count/sec
double
u_signif
Source significance for the filter U
sigma
double
u_sky_image
Source detected in stacked images filter U
char
u_srcdist
Dist. to the nearest source, U filter
arcsec
double
u_vega_mag
Source Vega magnitude for the filter U
mag
double
u_vega_mag_err
Source Vega magnitude error, filter U
mag
double
uvm2_ab_flux_err
Source flux error for the filter UVM2
erg/s/cm**2/A
double
uvm2_ab_mag
Source AB magnitude for the filter UVM2
mag
double
uvm2_ab_mag_err
Source AB magnitude error, filter UVM2
mag
double
uvm2_extended_flag
Source extended flag for the filter UVM2
int
uvm2_major_axis
Source major semi-axis for the filter UVM2
arcsec
double
uvm2_minor_axis
Source minor semi-axis for the filter UVM2
arcsec
double
uvm2_posang
Source position angle for the filter UVM2
degree
double
uvm2_quality_flag
Source quality flag for the filter UVM2
int
uvm2_quality_flag_st
Source quality flag string, filter UVM2
char
uvm2_rate
Source count rate for the filter UVM2
count/sec
double
uvm2_rate_err
Source count rate error, filter UVM2
count/sec
double
uvm2_signif
Source significance for the filter UVM2
sigma
double
uvm2_sky_image
Source detected in stacked images filter UVM2
char
uvm2_srcdist
Dist. to the nearest source, UVM2 filter
arcsec
double
uvm2_vega_mag
Source Vega magnitude for the filter UVM2
mag
double
uvm2_vega_mag_err
Source Vega magnitude error, filter UVM2
mag
double
uvw1_ab_flux_err
Source flux error for the filter UVW1
erg/s/cm**2/A
double
uvw1_ab_mag
Source AB magnitude for the filter UVW1
mag
double
uvw1_ab_mag_err
Source AB magnitude error, filter UVW1
mag
double
uvw1_extended_flag
Source extended flag for the filter UVW1
int
uvw1_major_axis
Source major semi-axis for the filter UVW1
arcsec
double
uvw1_minor_axis
Source minor semi-axis for the filter UVW1
arcsec
double
uvw1_posang
Source position angle for the filter UVW1
degree
double
uvw1_quality_flag
Source quality flag for the filter UVW1
int
uvw1_quality_flag_st
Source quality flag string, filter UVW1
char
uvw1_rate
Source count rate for the filter UVW1
count/sec
double
uvw1_rate_err
Source count rate error, filter UVW1
count/sec
double
uvw1_signif
Source significance for the filter UVW1
sigma
double
uvw1_sky_image
Source detected in stacked images filter UVW1
char
uvw1_srcdist
Dist. to the nearest source, UVW1 filter
arcsec
double
uvw1_vega_mag
Source Vega magnitude for the filter UVW1
mag
double
uvw1_vega_mag_err
Source Vega magnitude error, filter UVW1
mag
double
uvw2_ab_flux_err
Source flux error for the filter UVW2
erg/s/cm**2/A
double
uvw2_ab_mag
Source AB magnitude for the filter UVW2
mag
double
uvw2_ab_mag_err
Source AB magnitude error, filter UVW2
mag
double
uvw2_extended_flag
Source extended flag for the filter UVW2
int
uvw2_major_axis
Source major semi-axis for the filter UVW2
arcsec
double
uvw2_minor_axis
Source minor semi-axis for the filter UVW2
arcsec
double
uvw2_posang
Source position angle for the filter UVW2
degree
double
uvw2_quality_flag
Source quality flag for the filter UVW2
int
uvw2_quality_flag_st
Source quality flag string, filter UVW2
char
uvw2_rate
Source count rate for the filter UVW2
count/sec
double
uvw2_rate_err
Source count rate error, filter UVW2
count/sec
double
uvw2_signif
Source significance for the filter UVW2
sigma
double
uvw2_sky_image
Source detected in stacked images filter UVW2
char
uvw2_srcdist
Dist. to the nearest source, UVW2 filter
arcsec
double
uvw2_vega_mag
Source Vega magnitude for the filter UVW2
mag
double
uvw2_vega_mag_err
Source Vega magnitude error, filter UVW2
mag
double
v_ab_flux_err
Source flux error for the filter V
erg/s/cm**2/A
double
v_ab_mag
Source AB magnitude for the filter V
mag
double
v_ab_mag_err
Source AB magnitude error, filter V
mag
double
v_extended_flag
Source extended flag for the filter V
int
v_major_axis
Source major semi-axis for the filter V
arcsec
double
v_minor_axis
Source minor semi-axis for the filter V
arcsec
double
v_posang
Source position angle for the filter V
degree
double
v_quality_flag
Source quality flag for the filter V
int
v_quality_flag_st
Source quality flag string, filter V
char
v_rate
Source count rate for the filter V
count/sec
double
v_rate_err
Source count rate error, filter V
count/sec
double
v_signif
Source significance for the filter V
sigma
double
v_sky_image
Source detected in stacked images filter V
char
v_srcdist
Dist. to the nearest source, V filter
arcsec
double
v_vega_mag
Source Vega magnitude for the filter V
mag
double
v_vega_mag_err
Source Vega magnitude error, filter V
mag
double
iauname
Source IAU name
char
primary
observation_oid
int
primary
ra
Source Right Ascension coordinate (deg)
degrees
pos.eq.ra;meta.main
double
primary
dec
Source Declination coordinate (deg)
degrees
pos.eq.dec;meta.main
double
primary
poserr
Source positional (coordinate) error
arcsec
double
primary
uvw1_ab_flux
Source flux for the filter UVW1
erg/s/cm**2/A
double
primary
uvw2_ab_flux
Source flux for the filter UVW2
erg/s/cm**2/A
double
primary
uvm2_ab_flux
Source flux for the filter UVM2
erg/s/cm**2/A
double
primary
u_ab_flux
Source flux for the filter U
erg/s/cm**2/A
double
primary
v_ab_flux
Source flux for the filter V
erg/s/cm**2/A
double
primary
b_ab_flux
Source flux for the filter B
erg/s/cm**2/A
double
primary
catalogues.mv_xsa_slew_source_cat_fdw
altident
An alternative name for the best match source.
char
bg_map_b6
Background value for the soft band. (0.2-2.0 keV)
counts/pixel
double
bg_map_b7
Background value for the hard band. (2.0-12.0 keV)
counts/pixel
double
bg_map_b8
Background value for the total band. (0.2-12.0 keV)
counts/pixel
double
bii
Galactic Latitude [degrees]
deg
double
bii_b6
The galactic position in [degrees] of the soft band source. (0.2-2.0 keV)
deg
double
bii_b7
The galactic position in [degrees] of the hard band source. (2.0-12.0 keV)
deg
double
bii_b8
The galactic position in [degrees] of the total band source. (0.2-12.0 keV)
deg
double
date_end
SLEW exposure end date
char
date_obs
SLEW exposure start date
char
dec_b6
The J2000 celestial position of of the soft band source. (0.2-2.0 keV)
deg
double
dec_b7
The J2000 celestial position of of the hard band source. (2.0-12.0 keV)
deg
double
dec_b8
The J2000 celestial position of of the total band source. (0.2-12.0 keV)
deg
double
det_ml_b6
The detection likelihood in the soft (0.2-2.0 keV) energy band
double
det_ml_b7
The detection likelihood in the hard (2.0-12 keV) energy band
double
det_ml_b8
The detection likelihood in the total (0.2-12 keV) energy band
double
duration
Exposure on time
pixels
int
exp_map_b6
The effective on-axis exposure time in [seconds], in the soft energy band. (0.2-2.0 keV)
seconds
double
exp_map_b7
The effective on-axis exposure time in [seconds], in the hard energy band. (2.0-12.0 keV)
seconds
double
exp_map_b8
The effective on-axis exposure time in [seconds], in the total energy band. (0.2-12.0 keV)
seconds
double
ext_b6
Spatial extension of the source in the soft energy band. (0.2-2.0 keV)
pixels
double
ext_b6_err
Statistical one sigma error on the soft band extension parameter. (0.2-2.0 keV)
pixels
double
ext_b7
Spatial extension of the source in the hard energy band. (2.0-12.0 keV)
pixels
double
ext_b7_err
Statistical one sigma error on the hard band extension parameter. (2.0-12.0 keV)
pixels
double
ext_b8
Spatial extension of the source in the total energy band. (0.2-12.0 keV)
pixels
double
ext_b8_err
Statistical one sigma error on the total band extension parameter. (0.2-12.0 keV)
pixels
double
ext_ml_b6
Likelihood of the source being extended in the soft (0.2-2 keV) energy band
double
ext_ml_b7
Likelihood of the source being extended in the hard (2-12 keV) energy band
double
ext_ml_b8
Likelihood of the source being extended in the total (0.2-12 keV) energy band.
double
filt_cnts
The number of counts found within a 1 arcminute radius about the source position after standard filtering is applied.
double
flag_comment
A comment which explains why a particular source flag has been set to true
char
hr1
The hardness ratio, defined as HR1 = (rate_b7-rate_b6)/(rate_b7+rate_b6) where rate_b7 is the hard band count rate and rate_b6 is the soft band count rate. This has been calculated for the 1936 sources which have a positive detection in both bands
double
hr1_err
Error on the hardness ratio calculated as: sqrt(rate_b7_err*rate_b7_err + rate_b6_err*rate_b6_err) /(rate_b7+rate_b6) where rate_b7_err and rate_b6_err are the errors on the hard and soft band count rates respectively
double
id_category
The source type as returned by SIMBAD, NED and the other resources used in the cross-matching process.
char
id_dist
The distance in arcminutes between the best match candidate and the SLEW survey source
arcsec
double
ident
Cross-correlations of the positions of the slew sources with astronomical databases and catalogues have been performed (see section on IDs)
char
id_resource
The astronomical database or catalogue from which the best match has been selected.
char
image_bg_rate
Peak background count rate in the image from which the source was extracted
counts/s
double
lii
Galactic Longitude [degrees]
deg
double
lii_b6
The galactic position in [degrees] of the soft band source. (0.2-2.0 keV)
deg
double
lii_b7
The galactic position in [degrees] of the hard band source. (2.0-12.0 keV)
deg
double
lii_b8
The galactic position in [degrees] of the total band source. (0.2-12.0 keV)
deg
double
mjd_start
Modified Julian Date (i.e., JD - 2400000.5) of the start of the observation.
double
mjd_stop
Modified Julian Date (i.e., JD - 2400000.5) of the end of the observation.
double
mode_id
Observing mode of the EPIC-pn camera. FF= Full frame mode eFF = extended full frame mode LW = large window mode
char
npix
Healpix pixel of the center for nside 256
long
pos
char
postcard_url
meta.ref.url;meta.preview
char
ra_b6
The J2000 celestial position of the soft band source. (0.2-2.0 keV)
deg
double
ra_b7
The J2000 celestial position of the hard band source. (2.0-12.0 keV)
deg
double
ra_b8
The J2000 celestial position of the total band source. (0.2-12.0 keV)
deg
double
radec_b6_err
The statistical error in [degrees], on the soft band position. (0.2-2.0 keV)
deg
double
radec_b7_err
The statistical error in [degrees], on the hard band position. (2.0-12.0 keV)
deg
double
radec_b8_err
The statistical error in [degrees], on the total band position. (0.2-12.0 keV)
deg
double
radec_err
Radial error on the position, computed as sqrt(ra_err2 + dec_err2), in arcsecs, where ra_err and dec_err are the 1 sigma uncertainties in the RA and DEC coordinates respectively.
deg
double
rass_dist
The distance from the best match ROSAT source and the SLEW source
arcsec
double
rassname
char
rate_b6
The soft band count rate (0.2-2.0 keV)
counts/s
double
rate_b6_err
The error on the soft band count rate (0.2-2.0 keV)
counts/s
double
rate_b7
The hard band count rate (2.0-12.0 keV)
counts/s
double
rate_b7_err
The error on the hard band count rate (2.0-12.0 keV)
counts/s
double
rate_b8
The total band count rate (0.2-12.0 keV)
counts/s
double
rate_b8_err
The error on the total band count rate (0.2-12.0 keV)
counts/s
double
scts_b6
The number of background subtracted counts, in the soft energy band (0.2-2 keV), corrected for the PSF
counts
double
scts_b6_err
Statistical 1 sigma error on the soft band source counts (0.2-2.0 keV).
counts
double
scts_b7
The number of background subtracted counts, in the hard energy band (2.0-12.0 keV)
counts
double
scts_b7_err
Statistical 1 sigma error on the hard band source counts (2.0-12.0 keV)
counts
double
scts_b8
The number of background subtracted counts, in the total energy band (0.2-12.0 keV)
counts
double
scts_b8_err
Statistical 1 sigma error on the total band source counts (0.2-12.0 keV)
counts
double
slew_observation_id
SLEW observation ID
char
primary
slew_source_cat_fov_scircle
char
slew_source_cat_galactic_spoint
char
slew_source_cat_oid
int
srcname_b6
The source name defined in the soft band list. The format is 'xs' followed by the revolution number, the observation ID and the source position, e.g. xs0841_9084100002_12:57:07.5+01:50:42
char
srcname_b7
The source name defined in the hard band list. The format is 'xs' followed by the revolution number, the observation ID and the source position, e.g. xs0841_9084100002_12:57:07.5+01:50:42
char
srcname_b8
The source name defined in the total band list. The format is 'xs' followed by the revolution number, the observation ID and the source position, e.g. xs0841_9084100002_12:57:07.5+01:50:42
char
srcnum
This is the official name for sources detected in the XMM-Newton slew survey
int
unfilt_cnts
The number of counts found within a 1 arcminute radius about the source position with no filtering applied
double
us_extras
Name in the EXTRAS catalogue
double
us_xmmsl1
XMMSL1 name
char
val_flag
char
ver_false
This is a catch-all for problems not included in the other flags.
char
ver_halo
If set true, this flag indicates that a detection lies within the point spread function, or halo, of a very bright source and is probably spurious.
char
ver_hibgnd
If set true, this flag indicates that the source lies within a bright region, caused by high background, and is probably spurious.
char
ver_inext
If set true, this flag notes that a detection has been found within an extended source and is probably false. This flag is used to ensure that only one source is quoted for the large supernova remnants.
char
ver_nredg
Source near edge. Not used in XMMSL2.
char
ver_optload
A warning flag indicating that the source may suffer from optical loading
char
ver_psusp
This flag indicates that the quoted position of the source is likely to be inaccurate. In a few slews the attitude reconstruction is poor and in these cases the actual position of the source is difficult to determine and can be wrong by an arcminute.
char
x_ima_b6
The X position of the source in the soft band image in image pixels. (0.2-2.0 keV)
pixels
double
x_ima_b7
The X position of the source in the hard band image in image pixels. (2.0-12.0 keV)
pixels
double
x_ima_b8
The X position of the source in the total band image in image pixels. (0.2-12.0 keV)
pixels
double
ximname_b6
The name of the image containing the soft band detection. (0.2-2.0 keV)
char
ximname_b7
The name of the image containing the hard band detection. (2.0-12.0 keV)
char
ximname_b8
The name of the image containing the total band detection. (0.2-12.0 keV)
char
y_ima_b6
The Y position of the source in the soft band image in image pixels. (0.2-2.0 keV)
pixels
double
y_ima_b7
The Y position of the source in the hard band image in image pixels. (2.0-12.0 keV)
pixels
double
y_ima_b8
The Y position of the source in the total band image in image pixels. (0.2-12.0 keV)
pixels
double
name
meta.id;meta.main
char
primary
ra
Right Ascension [degrees]
deg
pos.eq.ra;meta.main
double
primary
dec
Declination J2000 [degrees]
deg
pos.eq.dec;meta.main
double
primary
flux_b8
The source flux in the total energy (0.2-12.0 keV)
(10E-12) ergs/s/cm2
double
primary
flux_b8_err
The error on the total band source flux.
(10E-12) ergs/s/cm2
double
primary
flux_b7
The source flux in the hard energy (2.0-12.0 keV)
(10E-12) ergs/s/cm2
double
primary
flux_b7_err
The error on the hard band source flux
(10E-12) ergs/s/cm2
double
primary
flux_b6
The source flux in the total energy (0.2-2.0 keV)
(10E-12) ergs/s/cm2
double
primary
flux_b6_err
The error on the soft band source flux
(10E-12) ergs/s/cm2
double
primary
catalogues.t_akari_point_source_catalogue_fdw
flags09
Bit flags data quality for S9W
char
flags18
Bit flags data quality for L18W
char
mconf09
Months confirmation flag for S9W
int
mconf18
Months confirmation flag for L18W
int
mean_ab09
Average of major and minor axes for S9W
arcsec
double
mean_ab18
Average of major and minor axes for L18W
arcsec
double
ndata_pos
Number of events used for positional calculation
int
ndens09
Number of neighboring sources for S9W
int
ndens18
Number of neighboring sources for L18W
int
nscanc09
nScanConfirm for S9W
int
nscanc18
nScanConfirm for L18W
int
nscanp09
nScanPossible for S9W
int
nscanp18
nScanPossible for L18W
int
poserrmi
Position error minor axis
arcsec
double
poserrmj
Position error major axis
arcsec
double
poserrpa
Position error Position Angle
deg
double
objname
Source Identifier
meta.id;meta.main
char
primary
ra
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
double
primary
dec
Declination (J2000)
deg
pos.eq.dec;meta.main
double
primary
flux09
Flux density in S9W
Jy
double
primary
ferr09
Flux error in S9W
Jy
double
primary
flux18
Flux density in L18W
Jy
double
primary
ferr18
Flux error in L18W
Jy
double
primary
fqual09
Flux quality flag for S9W
int
primary
fqual18
Flux quality flag for L18W
int
primary
extended09
Extended source flag for S9W
int
primary
extended18
Extended source flag for L18W
int
primary
ndata09
Number of events contributing to FLUX09
int
primary
ndata18
Number of events contributing to FLUX18
int
primary
catalogues.t_allwise_original_valid_fdw
ext_flag
Extended source flag. This is an integer flag, the value of which indicates whether or not the morphology of a source is consistent with the WISE point spread function in any band, or whether the source is associated with or superimposed on a previously known extended object from the 2MASS Extended Source Catalog (XSC). The values of the extFlag indicate the following conditions: - 0 - The source shape is consistent with a point-source and the source is not associated with or superimposed on a 2MASS XSC source - 1 - The profile-fit photometry goodness-of-fit is >3.0 in one or more bands. - 2 - The source falls within the extrapolated isophotal footprint of a 2MASS XSC source. - 3 - The profile-fit photometry goodness-of-fit is >3.0 in one or more bands, and the source falls within the extrapolated isophotal footprint of a 2MASS XSC source. - 4 - The source position falls within 5 arcsec of a 2MASS XSC source. - 5 - The profile-fit photometry goodness-of-fit is >3.0 in one or more bands, and the source position falls within 5 arcsec of a 2MASS XSC source. CAUTION: WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
short
w1gmag
W1 magnitude of source measured in the elliptical aperture. WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
mag
double
w1gmag_error
Uncertainty in the W1 magnitude of source measured in elliptical aperture. CAUTION: A w1gerr value of 9.999 indicates that the measurement uncertainty is very large, or the uncertainty could not be computed. In either case, the w1gmag measurement should be considered highly suspect.
mag
double
w1mjd_mean
The average modified Julian Date (mJD) of the W1 single-exposures covering the source.
d
double
w2gmag
W2 magnitude of source measured in the elliptical aperture. WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
mag
double
w2mjd_mean
The average modified Julian Date (mJD) of the W2 single-exposures covering the source.
d
double
w3gmag
W3 magnitude of source measured in the elliptical aperture. WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
mag
double
w3gmag_error
Uncertainty in the W3 magnitude of source measured in elliptical aperture. CAUTION: A w3gerr value of 9.999 indicates that the measurement uncertainty is very large, or the uncertainty could not be computed. In either case, the w3gmag measurement should be considered highly suspect.
mag
double
w3mjd_mean
The average modified Julian Date (mJD) of the W3 single-exposures covering the source.
d
double
w4gmag
W4 magnitude of source measured in the elliptical aperture. WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
mag
double
w4gmag_error
Uncertainty in the W4 magnitude of source measured in elliptical aperture. CAUTION: A w4gError value of 9.999 indicates that the measurement uncertainty is very large, or the uncertainty could not be computed. In either case, the w4gmag measurement should be considered highly suspect.
mag
double
w4mjd_mean
The average modified Julian Date (mJD) of the W4 single-exposures covering the source.
d
double
name
AllWISE name. Sexagesimal, equatorial position-based source name in the form: hhmmss.ss+ddmmss.s. The full naming convention for AllWISE Source Catalog sources has the form “WISEA Jhhmmss.ss+ddmmss.s,” where “WISEA” indicates the source is from the AllWISE Source Catalog, and “J” indicates the position is J2000. The “WISEA” acronym is not listed explicitly in the designation column.
meta.id;meta.main
char
primary
ra
J2000 right ascension with respect to the 2MASS PSC reference frame from the non-moving source extraction. The sky coverage depth for sources in the AllWISE Catalog is approximately twice as large in W1 and W2 as it is in W3 and W4. AllWISE combined W1 and W2 Single-exposure images from the WISE 4-Band Cryo, 3-Band Cryo and NEOWISE Post-Cryo survey phases, and W3 and W4 images from the 4-Band Cryo phase only. The additional epoch of W1 and W2 coverage accenuates the weight of those two bands in determining source properties such as position and motion.
deg
pos.eq.ra;meta.main
double
primary
dec
J2000 declination with respect to the 2MASS PSC reference frame from the non-moving source extraction. The sky coverage depth for sources in the AllWISE Catalog is approximately twice as large in W1 and W2 as it is in W3 and W4. AllWISE combined W1 and W2 Single-exposure images from the WISE 4-Band Cryo, 3-Band Cryo and NEOWISE Post-Cryo survey phases, and W3 and W4 images from the 4-Band Cryo phase only. The additional epoch of W1 and W2 coverage accenuates the weight of those two bands in determining source properties such as position and motion.
deg
pos.eq.dec;meta.main
double
primary
ra_error
One-sigma uncertainty in right ascension coordinate from the non-moving source extraction.
arcsec
double
primary
dec_error
One-sigma uncertainty in declination coordinate from the non-moving source extraction.
arcsec
double
primary
w1mpro
W1 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W1 flux measurement has SNR<2. This column is null if the source is nominally detected in W1, but no useful brightness estimate could be made. The corresponding error column is null if the W1 profile-fit magnitude is a 95% confidence upper limit. CAUTION: WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
mag
double
primary
w1mpro_error
W1 profile-fit photometric measurement uncertainty in mag units. This column is null if the W1 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.
mag
double
primary
w2mpro
W2 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W2 flux measurement has SNR<2. This column is null if the source is nominally detected in W2, but no useful brightness estimate could be made. The corresponding error column is null if the W2 profile-fit magnitude is a 95% confidence upper limit. CAUTION: WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
mag
double
primary
w2mpro_error
W2 profile-fit photometric measurement uncertainty in mag units. This column is null if the W2 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.
mag
double
primary
w3mpro
W3 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W3 flux measurement has SNR<2. This column is null if the source is nominally detected in W3, but no useful brightness estimate could be made. The corresponding error column is null if the W3 profile-fit magnitude is a 95% confidence upper limit. CAUTION: WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
mag
double
primary
w3mpro_error
W3 profile-fit photometric measurement uncertainty in mag units. This column is null if the W3 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.
mag
double
primary
w4mpro
W4 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W4 flux measurement has SNR<2. This column is null if the source is nominally detected in W4, but no useful brightness estimate could be made. The corresponding error column is null if the W1 profile-fit magnitude is a 95% confidence upper limit. CAUTION: WISE profile-fit (w?mpro) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has extFlag>0, you may wish to examine the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies.
mag
double
primary
w4mpro_error
W4 profile-fit photometric measurement uncertainty in mag units. This column is null if the W4 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.
mag
double
primary
catalogues.t_gaiafpr_crowded_field_source_fdw
designation
Unique source designation (unique across all Data Releases)
meta.id;meta.main
char
primary
region_name
Name of the designated CrowdedField region in the sky
meta.id
char
source_id
Unique source identifier (unique within a particular Data Release) providing the CrowdedField-nature of the source via location bit
meta.id
char
primary
ref_epoch
Reference epoch
yr
meta.ref;time.epoch
stc:AstroCoords.Time.TimeInstant
double
ra
Right ascension
deg
pos.eq.ra;meta.main
stc:AstroCoords.Position3D.Value3.C1
double
primary
ra_error
Standard error of right ascension
mas
stat.error;pos.eq.ra
stc:AstroCoords.Position3D.Error3.C1
float
dec
Declination
deg
pos.eq.dec;meta.main
stc:AstroCoords.Position3D.Value3.C2
double
primary
dec_error
Standard error of declination
mas
stat.error;pos.eq.dec
stc:AstroCoords.Position3D.Error3.C2
float
parallax
Parallax
mas
pos.parallax.trig
double
primary
parallax_error
Standard error of parallax
mas
stat.error;pos.parallax.trig
float
primary
parallax_over_error
Parallax divided by its standard error
stat.snr;pos.parallax.trig
float
pm
Total proper motion
mas.yr**-1
pos.pm;pos.eq
float
pmra
Proper motion in right ascension direction
mas.yr**-1
pos.pm;pos.eq.ra
stc:AstroCoords.Velocity3D.Value3.C1
double
primary
pmra_error
Standard error of proper motion in right ascension direction
mas.yr**-1
stat.error;pos.pm;pos.eq.ra
stc:AstroCoords.Velocity3D.Error3.C1
float
primary
pmdec
Proper motion in declination direction
mas.yr**-1
pos.pm;pos.eq.dec
stc:AstroCoords.Velocity3D.Value3.C2
double
primary
pmdec_error
Standard error of proper motion in declination direction
mas.yr**-1
stat.error;pos.pm;pos.eq.dec
stc:AstroCoords.Velocity3D.Error3.C2
float
primary
ra_dec_corr
Correlation between right ascension and declination
stat.correlation
float
ra_parallax_corr
Correlation between right ascension and parallax
stat.correlation
float
ra_pmra_corr
Correlation between right ascension and proper motion in right ascension
stat.correlation
float
ra_pmdec_corr
Correlation between right ascension and proper motion in declination
stat.correlation
float
dec_parallax_corr
Correlation between declination and parallax
stat.correlation
float
dec_pmra_corr
Correlation between declination and proper motion in right ascension
stat.correlation
float
dec_pmdec_corr
Correlation between declination and proper motion in declination
stat.correlation
float
parallax_pmra_corr
Correlation between parallax and proper motion in right ascension
stat.correlation
float
parallax_pmdec_corr
Correlation between parallax and proper motion in declination
stat.correlation
float
pmra_pmdec_corr
Correlation between proper motion in right ascension and proper motion in declination
stat.correlation
float
n_scans
Number of CrowdedField scans of the source location
meta.number
short
astrometric_n_obs_al
Total number of observations in the along-scan (AL) direction
meta.number
short
astrometric_n_obs_ac
Total number of observations in the across-scan (AC) direction
meta.number
short
astrometric_n_good_obs_al
Number of good observations in the along-scan (AL) direction
meta.number
short
astrometric_n_bad_obs_al
Number of bad observations in the along-scan (AL) direction
meta.number
short
astrometric_gof_al
Goodness of fit statistic of model wrt along-scan observations
stat.fit.goodness
float
astrometric_chi2_al
AL chi-square value
stat.fit.chi2
float
astrometric_excess_noise
Excess noise of the source
mas
stat.value
float
astrometric_excess_noise_sig
Significance of excess noise
stat.value
float
astrometric_params_solved
Which parameters have been solved for?
meta.number
short
pseudocolour
Astrometrically estimated pseudocolour of the source
um**-1
em.wavenumber
float
pseudocolour_error
Standard error of the pseudocolour of the source
um**-1
stat.error;em.wavenumber
float
ra_pseudocolour_corr
Correlation between right ascension and pseudocolour
stat.correlation;em.wavenumber;pos.eq.ra
float
dec_pseudocolour_corr
Correlation between declination and pseudocolour
stat.correlation;em.wavenumber;pos.eq.dec
float
parallax_pseudocolour_corr
Correlation between parallax and pseudocolour
stat.correlation;em.wavenumber;pos.parallax
float
pmra_pseudocolour_corr
Correlation between proper motion in right asension and pseudocolour
stat.correlation;em.wavenumber;pos.pm;pos.eq.ra
float
pmdec_pseudocolour_corr
Correlation between proper motion in declination and pseudocolour
stat.correlation;em.wavenumber;pos.pm;pos.eq.dec
float
astrometric_matched_transits
Matched FOV transits used in the AGIS solution
meta.number
short
visibility_periods_used
Number of visibility periods used in Astrometric solution
meta.number
short
astrometric_sigma5d_max
The longest semi-major axis of the 5-d error ellipsoid
mas
stat;pos.errorEllipse
float
matched_transits
The number of transits matched to this source
meta.number
short
ipd_gof_harmonic_amplitude
Amplitude of the IPD GoF versus position angle of scan
stat.value
float
ipd_gof_harmonic_phase
Phase of the IPD GoF versus position angle of scan
deg
pos.posAng;stat.value
float
scan_direction_strength_k1
Degree of concentration of scan directions across the source
stat.value
float
scan_direction_strength_k2
Degree of concentration of scan directions across the source
stat.value
float
scan_direction_strength_k3
Degree of concentration of scan directions across the source
stat.value
float
scan_direction_strength_k4
Degree of concentration of scan directions across the source
stat.value
float
scan_direction_mean_k1
Mean position angle of scan directions across the source
deg
pos.posAng;stat.mean
float
scan_direction_mean_k2
Mean position angle of scan directions across the source
deg
pos.posAng;stat.mean
float
scan_direction_mean_k3
Mean position angle of scan directions across the source
deg
pos.posAng;stat.mean
float
scan_direction_mean_k4
Mean position angle of scan directions across the source
deg
pos.posAng;stat.mean
float
astrometric_primary_flag
Primary or secondary
meta.code
boolean
phot_g_n_obs
Number of observations contributing to G photometry
meta.number
short
phot_g_mean_flux
G-band mean flux
electron.s**-1
phot.flux;em.opt
double
phot_g_mean_flux_error
Error on G-band mean flux
electron.s**-1
stat.error;phot.flux;em.opt
float
phot_g_mean_flux_over_error
G-band mean flux divided by its error
stat.snr;phot.flux;em.opt
float
phot_g_mean_mag
G-band mean magnitude
mag
phot.mag;em.opt
float
primary
phot_g_flux_uwv
Unit weight variance of fluxes
stat.weight
double
phot_g_flux_median
Median flux
electron.s**-1
phot.flux;stat.median
float
phot_g_flux_skewness
Measure of the skewness of the flux distribution
phot.flux;stat.value
float
phot_g_flux_kurtosis
Measure of the kurtosis of the flux distribution
phot.flux;stat.value
float
phot_g_flux_mad
MAD of the flux distribution
electron.s**-1
phot.flux;stat.value
float
phot_g_flux_first_quartile
First quartile of the flux distribution
electron.s**-1
phot.flux;stat.value
float
phot_g_flux_third_quartile
Third quartile of the flux distribution
electron.s**-1
phot.flux;stat.value
float
phot_g_flux_min
Minimum flux value
electron.s**-1
phot.flux;stat.min
float
phot_g_flux_max
Maximum flux value
electron.s**-1
phot.flux;stat.max
float
phot_proc_mode
Photometry processing mode
meta.code
short
l
Galactic longitude
deg
pos.galactic.lon
stc:AstroCoords.Position2D.Value2.C1
double
b
Galactic latitude
deg
pos.galactic.lat
stc:AstroCoords.Position2D.Value2.C2
double
ecl_lon
Ecliptic longitude
deg
pos.ecliptic.lon
stc:AstroCoords.Position2D.Value2.C1
double
ecl_lat
Ecliptic latitude
deg
pos.ecliptic.lat
stc:AstroCoords.Position2D.Value2.C2
double
catalogues.t_gaia_source_dr3_fdw
ag_gspphot_lower
Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra
mag
phys.absorption;em.opt
float
ag_gspphot_upper
Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra
mag
phys.absorption;em.opt
float
astrometric_chi2_al
AL chi-square value
stat.fit.chi2
float
astrometric_excess_noise
Excess noise of the source
mas
stat.value
float
astrometric_excess_noise_sig
Significance of excess noise
stat.value
float
astrometric_gof_al
Goodness of fit statistic of model wrt along-scan observations
stat.fit.goodness
float
astrometric_matched_transits
Matched FOV transits used in the AGIS solution
meta.number
short
astrometric_n_bad_obs_al
Number of bad observations in the along-scan (AL) direction
meta.number
short
astrometric_n_good_obs_al
Number of good observations in the along-scan (AL) direction
meta.number
short
astrometric_n_obs_ac
Total number of observations in the across-scan (AC) direction
meta.number
short
astrometric_n_obs_al
Total number of observations in the along-scan (AL) direction
meta.number
short
astrometric_params_solved
Which parameters have been solved for?
meta.number
short
astrometric_primary_flag
Primary or seconday
meta.code
boolean
astrometric_sigma5d_max
The longest semi-major axis of the 5-d error ellipsoid
mas
stat;pos.errorEllipse
float
azero_gspphot_lower
Lower confidence level (16%) of monochromatic extinction $A_0$ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra
mag
phys.absorption;em.opt
float
azero_gspphot_upper
Upper confidence level (84%) of monochromatic extinction $A_0$ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra
mag
phys.absorption;em.opt
float
b
Galactic latitude
deg
pos.galactic.lat
stc:AstroCoords.Position2D.Value2.C2
double
classprob_dsc_combmod_galaxy
Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)
stat.probability
float
classprob_dsc_combmod_quasar
Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)
stat.probability
float
classprob_dsc_combmod_star
Probability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum, photometry, astrometry)
stat.probability
float
dec_error
Standard error of declination
mas
stat.error;pos.eq.dec
stc:AstroCoords.Position3D.Error3.C2
float
dec_parallax_corr
Correlation between declination and parallax
stat.correlation
float
dec_pmdec_corr
Correlation between declination and proper motion in declination
stat.correlation
float
dec_pmra_corr
Correlation between declination and proper motion in right ascension
stat.correlation
float
dec_pseudocolour_corr
Correlation between declination and pseudocolour
stat.correlation;em.wavenumber;pos.eq.dec
float
distance_gspphot_lower
Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra
pc
pos.distance;pos.eq
float
distance_gspphot_upper
Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra
pc
pos.distance;pos.eq
float
duplicated_source
Source with multiple source identifiers
meta.code.status
boolean
ebpminrp_gspphot_lower
Lower confidence level (16%) of reddening $E(G_{\rm BP} - G_{\rm RP})$ from GSP-Phot Aeneas best library using BP/RP spectra
mag
phot.color.excess;stat.min
float
ebpminrp_gspphot_upper
Upper confidence level (84%) of reddening $E(G_{\rm BP} - G_{\rm RP})$ from GSP-Phot Aeneas best library using BP/RP spectra
mag
phot.color.excess;stat.max
float
ecl_lat
Ecliptic latitude
deg
pos.ecliptic.lat
stc:AstroCoords.Position2D.Value2.C2
double
ecl_lon
Ecliptic longitude
deg
pos.ecliptic.lon
stc:AstroCoords.Position2D.Value2.C1
double
grvs_mag
Integrated Grvs magnitude
mag
phot.mag;em.opt
stc:AstroCoords.Velocity3D.Value3.C3
float
grvs_mag_error
Grvs magnitude uncertainty
mag
stat.error;phot.mag;em.opt
stc:AstroCoords.Velocity3D.Error3.C3
float
grvs_mag_nb_transits
Number of transits used to compute Grvs
meta.number
short
has_epoch_rv
Flag indicating the availability of epoch radial velocity for this source
meta.code.status
boolean
in_andromeda_survey
Flag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS)
meta.code.status
boolean
in_galaxy_candidates
Flag indicating the availability of additional information in the galaxy candidates table
meta.code.status
boolean
in_qso_candidates
Flag indicating the availability of additional information in the QSO candidates table
meta.code.status
boolean
ipd_frac_multi_peak
Percent of successful-IPD windows with more than one peak
stat.value
short
ipd_frac_odd_win
Percent of transits with truncated windows or multiple gate
stat.value
short
ipd_gof_harmonic_amplitude
Amplitude of the IPD GoF versus position angle of scan
stat.value
float
ipd_gof_harmonic_phase
Phase of the IPD GoF versus position angle of scan
deg
pos.posAng;stat.value
float
l
Galactic longitude
deg
pos.galactic.lon
stc:AstroCoords.Position2D.Value2.C1
double
libname_gspphot
Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table
meta.note
char
logg_gspphot_lower
Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra
log(cm.s**-2)
phys.gravity;stat.min
float
logg_gspphot_upper
Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra
log(cm.s**-2)
phys.gravity;stat.max
float
matched_transits
The number of transits matched to this source
meta.number
short
matched_transits_removed
The number of transits removed from an existing source in the current cycle
meta.number
short
mh_gspphot_lower
Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra
'dex'
phys.abund.Z;stat.min
float
mh_gspphot_upper
Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra
'dex'
phys.abund.Z;stat.max
float
new_matched_transits
The number of transits newly incorporated into an existing source in the current cycle
meta.number
short
npix
int
nu_eff_used_in_astrometry
Effective wavenumber of the source used in the astrometric solution
um**-1
em.wavenumber
float
parallax_over_error
Parallax divided by its standard error
stat.snr;pos.parallax.trig
float
parallax_pmdec_corr
Correlation between parallax and proper motion in declination
stat.correlation
float
parallax_pmra_corr
Correlation between parallax and proper motion in right ascension
stat.correlation
float
parallax_pseudocolour_corr
Correlation between parallax and pseudocolour
stat.correlation;em.wavenumber;pos.parallax
float
phot_bp_mean_flux
Integrated BP mean flux
'electron'.s**-1
phot.flux;em.opt.B
double
phot_bp_mean_flux_error
Error on the integrated BP mean flux
'electron'.s**-1
stat.error;phot.flux;em.opt.B
float
phot_bp_mean_flux_over_error
Integrated BP mean flux divided by its error
stat.snr;phot.flux;em.opt.B
float
phot_bp_n_blended_transits
Number of BP blended transits
meta.number
short
phot_bp_n_contaminated_transits
Number of BP contaminated transits
meta.number
short
phot_bp_n_obs
Number of observations contributing to BP photometry
meta.number
short
phot_bp_rp_excess_factor
BP/RP excess factor
arith.factor;phot.flux;em.opt
float
phot_g_mean_flux
G-band mean flux
'electron'.s**-1
phot.flux;em.opt
double
phot_g_mean_flux_error
Error on G-band mean flux
'electron'.s**-1
stat.error;phot.flux;em.opt
float
phot_g_mean_flux_over_error
G-band mean flux divided by its error
stat.snr;phot.flux;em.opt
float
phot_g_n_obs
Number of observations contributing to G photometry
meta.number
short
phot_proc_mode
Photometry processing mode
meta.code
short
phot_rp_mean_flux
Integrated RP mean flux
'electron'.s**-1
phot.flux;em.opt.R
double
phot_rp_mean_flux_error
Error on the integrated RP mean flux
'electron'.s**-1
stat.error;phot.flux;em.opt.R
float
phot_rp_mean_flux_over_error
Integrated RP mean flux divided by its error
stat.snr;phot.flux;em.opt.R
float
phot_rp_n_blended_transits
Number of RP blended transits
meta.number
short
phot_rp_n_contaminated_transits
Number of RP contaminated transits
meta.number
short
phot_rp_n_obs
Number of observations contributing to RP photometry
meta.number
short
pm
Total proper motion
mas.yr**-1
pos.pm;pos.eq
float
pmdec_pseudocolour_corr
Correlation between proper motion in declination and pseudocolour
stat.correlation;em.wavenumber;pos.pm;pos.eq.dec
float
pmra_pmdec_corr
Correlation between proper motion in right ascension and proper motion in declination
stat.correlation
float
pmra_pseudocolour_corr
Correlation between proper motion in right asension and pseudocolour
stat.correlation;em.wavenumber;pos.pm;pos.eq.ra
float
pseudocolour
Astrometrically estimated pseudocolour of the source
um**-1
em.wavenumber
float
pseudocolour_error
Standard error of the pseudocolour of the source
um**-1
stat.error;em.wavenumber
float
ra_dec_corr
Correlation between right ascension and declination
stat.correlation
float
ra_error
Standard error of right ascension
mas
stat.error;pos.eq.ra
stc:AstroCoords.Position3D.Error3.C1
float
random_index
Random index for use when selecting subsets
meta.code
long
ra_parallax_corr
Correlation between right ascension and parallax
stat.correlation
float
ra_pmdec_corr
Correlation between right ascension and proper motion in declination
stat.correlation
float
ra_pmra_corr
Correlation between right ascension and proper motion in right ascension
stat.correlation
float
ra_pseudocolour_corr
Correlation between right ascension and pseudocolour
stat.correlation;em.wavenumber;pos.eq.ra
float
ref_epoch
Reference epoch
yr
meta.ref;time.epoch
stc:AstroCoords.Time.TimeInstant
double
rv_amplitude_robust
Total amplitude in the radial velocity time series after outlier removal
km.s**-1
stat.error;spect.dopplerVeloc.opt;em.opt.I
float
rv_atm_param_origin
Origin of the atmospheric parameters associated to the template
meta.code.class
short
rv_chisq_pvalue
P-value for constancy based on a chi-squared criterion
stat.fit.param
float
rv_expected_sig_to_noise
Expected signal to noise ratio in the combination of the spectra used to obtain the radial velocity
stat.snr
float
rv_method_used
Method used to obtain the radial velocity
meta.code.class
short
rv_nb_deblended_transits
Number of valid transits that have undergone deblending
meta.number
short
rv_nb_transits
Number of transits used to compute the radial velocity
meta.number
short
rv_renormalised_gof
Radial velocity renormalised goodness of fit
stat.fit.goodness
float
rvs_spec_sig_to_noise
Signal to noise ratio in the mean RVS spectrum
stat.snr
float
rv_template_fe_h
[Fe/H] of the template used to compute the radial velocityy
'dex'
stat.fit.param
float
rv_template_logg
Logg of the template used to compute the radial velocity
log(cm.s**-2)
stat.fit.param
float
rv_template_teff
Teff of the template used to compute the radial velocity
K
stat.fit.param
float
rv_time_duration
Time coverage of the radial velocity time series
d
time.duration
float
rv_visibility_periods_used
Number of visibility periods used to estimate the radial velocity
meta.number
short
scan_direction_mean_k1
Mean position angle of scan directions across the source
deg
pos.posAng;stat.mean
float
scan_direction_mean_k2
Mean position angle of scan directions across the source
deg
pos.posAng;stat.mean
float
scan_direction_mean_k3
Mean position angle of scan directions across the source
deg
pos.posAng;stat.mean
float
scan_direction_mean_k4
Mean position angle of scan directions across the source
deg
pos.posAng;stat.mean
float
scan_direction_strength_k1
Degree of concentration of scan directions across the source
stat.value
float
scan_direction_strength_k2
Degree of concentration of scan directions across the source
stat.value
float
scan_direction_strength_k3
Degree of concentration of scan directions across the source
stat.value
float
scan_direction_strength_k4
Degree of concentration of scan directions across the source
stat.value
float
solution_id
Solution Identifier
meta.version
long
source_id
Unique source identifier (unique within a particular Data Release)
meta.id
char
teff_gspphot_lower
Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra
K
phys.temperature.effective;stat.min
float
teff_gspphot_upper
Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra
K
phys.temperature.effective;stat.max
float
vbroad
Spectral line broadening parameter
km.s**-1
spect.dopplerVeloc.opt;em.opt.I
stc:AstroCoords.Velocity3D.Value3.C3
float
vbroad_error
Uncertainty on the spectral line broadening
km.s**-1
stat.error;spect.dopplerVeloc.opt;em.opt.I
stc:AstroCoords.Velocity3D.Error3.C3
float
vbroad_nb_transits
Number of transits used to compute vbroad
meta.number
short
visibility_periods_used
Number of visibility periods used in Astrometric solution
meta.number
short
designation
Unique source designation (unique across all Data Releases)
meta.id;meta.main
char
primary
ra
Right ascension
deg
pos.eq.ra;meta.main
stc:AstroCoords.Position3D.Value3.C1
double
primary
dec
Declination
deg
pos.eq.dec;meta.main
stc:AstroCoords.Position3D.Value3.C2
double
primary
parallax
Parallax
mas
pos.parallax.trig
double
primary
parallax_error
Standard error of parallax
mas
stat.error;pos.parallax.trig
float
primary
pmra
Proper motion in right ascension direction
mas.yr**-1
pos.pm;pos.eq.ra
stc:AstroCoords.Velocity3D.Value3.C1
double
primary
pmra_error
Standard error of proper motion in right ascension direction
mas.yr**-1
stat.error;pos.pm;pos.eq.ra
stc:AstroCoords.Velocity3D.Error3.C1
float
primary
pmdec
Proper motion in declination direction
mas.yr**-1
pos.pm;pos.eq.dec
stc:AstroCoords.Velocity3D.Value3.C2
double
primary
pmdec_error
Standard error of proper motion in declination direction
mas.yr**-1
stat.error;pos.pm;pos.eq.dec
stc:AstroCoords.Velocity3D.Error3.C2
float
primary
phot_g_mean_mag
G-band mean magnitude
mag
phot.mag;em.opt
float
primary
phot_bp_mean_mag
Integrated BP mean magnitude
mag
phot.mag;em.opt.B
float
primary
phot_rp_mean_mag
Integrated RP mean magnitude
mag
phot.mag;em.opt.R
float
primary
phot_variable_flag
Photometric variability flag
meta.code;src.var
char
primary
bp_rp
BP - RP colour
mag
phot.color;em.opt.B;em.opt.R
float
primary
bp_g
BP - G colour
mag
phot.color;em.opt.B;em.opt
float
primary
g_rp
G - RP colour
mag
phot.color;em.opt;em.opt.R
float
primary
radial_velocity
Radial velocity
km.s**-1
spect.dopplerVeloc.opt;em.opt.I
stc:AstroCoords.Velocity3D.Value3.C3
float
primary
radial_velocity_error
Radial velocity error
km.s**-1
stat.error;spect.dopplerVeloc.opt;em.opt.I
stc:AstroCoords.Velocity3D.Error3.C3
float
primary
ruwe
Renormalised unit weight error
stat.error
float
primary
non_single_star
Flag indicating the availability of additional information in the various Non-Single Star tables
meta.code.status
short
primary
has_xp_continuous
Flag indicating the availability of mean BP/RP spectrum in continuous representation for this source
meta.code.status
boolean
primary
has_xp_sampled
Flag indicating the availability of mean BP/RP spectrum in sampled form for this source
meta.code.status
boolean
primary
has_rvs
Flag indicating the availability of mean RVS spectrum for this source
meta.code.status
boolean
primary
has_epoch_photometry
Flag indicating the availability of epoch photometry for this source
meta.code.status
boolean
primary
has_mcmc_gspphot
Flag indicating the availability of GSP-Phot MCMC samples for this source
meta.code.status
boolean
primary
has_mcmc_msc
Flag indicating the availability of MSC MCMC samples for this source
meta.code.status
boolean
primary
teff_gspphot
Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra
K
phys.temperature.effective
float
primary
logg_gspphot
Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra
log(cm.s**-2)
phys.gravity
float
primary
mh_gspphot
Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra
'dex'
phys.abund.Z
float
primary
distance_gspphot
Distance from GSP-Phot Aeneas best library using BP/RP spectra
pc
pos.distance;pos.eq
float
primary
azero_gspphot
Monochromatic extinction $A_0$ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra
mag
phys.absorption;em.opt
float
primary
ag_gspphot
Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra
mag
phys.absorption;em.opt
float
primary
ebpminrp_gspphot
Reddening $E(G_{\rm BP} - G_{\rm RP})$ from GSP-Phot Aeneas best library using BP/RP spectra
mag
phot.color.excess
float
primary
catalogues.t_tmass_original_valid_fdw
err_ang
Position angle on the sky of the semi-major axis of the position uncertainty ellipse (East of North)
deg
int
err_maj
Semi-major axis length of the one sigma position uncertainty ellipse
arcsec
float
err_min
Semi-minor axis length of the one sigma position uncertainty ellipse
arcsec
float
ext_key
Unique identification number of the record in the XSC (2MASS Extended Source Catalogue) that corresponds to this point source. Can be NULL if no corresponding extended source is present in the XSC.
long
j_date
The Julian Date of the source measurement accurate to +30 seconds. This value is extrapolated from the start time of the Survey scan using the difference between the declinations of the source and the first row in the Tile divided by the scanning rate of the telescope (approximately 5sec). The scanning rate of the two 2MASS telescopes was slightly different because of the need to optimize the dithering of images on the arrays.
d
double
name
2MASS name. Sexagesimal, equatorial position-based source name in the form: Jhmmssss+ddmmsss[ABC...] The prefix “2MASS ” is not explicitly listed in the designation.
meta.id;meta.main
char
primary
ra
J2000 right ascension with respect to the ICRS
deg
pos.eq.ra;meta.main
double
primary
dec
J2000 declination with respect to the ICRS
deg
pos.eq.dec;meta.main
double
primary
j_m
Default J-band magnitude. In the case of a source not detected in the J-band, it is an upper limit and the corresponding total photometric uncertainty is NULL. In the case of a source detected in the J-band and with no useful brightness estimate, it is set to NULL.
mag
float
primary
j_msigcom
Total photometric uncertainty for the default J-band magnitude. This column is NULL if the default magnitude is a 95% confidence upper limit (i.e. the source is not detected, or inconsistently deblended in the J-band).
mag
float
primary
h_m
Default H-band magnitude. In the case of a source not detected in the H-band, it is an upper limit and the corresponding total photometric uncertainty is NULL. In the case of a source detected in the H-band and with no useful brightness estimate, it is set to NULL.
mag
float
primary
h_msigcom
Total photometric uncertainty for the default H-band magnitude. This column is NULL if the default magnitude is a 95% confidence upper limit (i.e. the source is not detected, or inconsistently deblended in the H-band).
mag
float
primary
ks_m
Default Ks-band magnitude. In the case of a source not detected in the Ks-band, it is an upper limit and the corresponding total photometric uncertainty is NULL. In the case of a source detected in the Ks-band and with no useful brightness estimate, it is set to NULL.
mag
float
primary
ks_msigcom
Total photometric uncertainty for the default Ks-band magnitude. This column is NULL if the default magnitude is a 95% confidence upper limit (i.e. the source is not detected, or inconsistently deblended in the Ks-band.
mag
float
primary
catalogues.t_v_akari_asteroids_flux_cat_fdw
alpha
Phase angle (Sun-Target-Observer angle)
deg
double
a_name
Asteroid name
char
a_num
Asteroid number
int
bn
Observed band
int
ccflux
Color-corrected flux density
Jy
double
cit
Reference
char
clat
char
clon
char
datetime
Observation date and time
char
dec
Declination (J2000) in decimal degrees
deg
pos.eq.dec;meta.main
double
delta
AKARI-centric distance
AU
double
e_ccflux
Color-corrected flux density uncertainty
Jy
double
e_influx
In-band flux density uncertainty
Jy
double
elong
Elongation angle (Sun-Observer-Target angle)
deg
double
influx
In-band flux density
Jy
double
naif_id
NAIF ID
int
oid
int
o_mode
Observational mode
char
prov_des
Provisional designation
char
ra
Right ascension (J2000) in decimal degrees
deg
pos.eq.ra;meta.main
double
rh
Heliocentric distance
AU
double
images
images.euclid_outreach
credit
char
description
char
euclid_outreach_oid
meta.oid
int
fov_size
double
id
meta.id;meta.main
char
large_url
char
pixel_size
char
priority
int
rotation
double
stc_s
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
char
fov
pos.outline;meta.pgsphere
char
npix
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
char
primary
title
char
primary
images.hst_outreach
credit
char
description
char
fov_size
double
hst_outreach_oid
meta.oid
int
id
meta.id;meta.main
char
large_url
char
pixel_size
char
priority
int
rotation
double
stc_s
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
char
fov
pos.outline;meta.pgsphere
char
npix
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
char
primary
title
char
primary
images.mv_euclid_outreach_ext_fdw
credit
char
description
char
euclid_outreach_oid
meta.oid
int
fov_size
double
id
meta.id;meta.main
char
large_url
char
pixel_size
char
priority
int
rotation
double
stc_s
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
char
primary
title
char
primary
images.mv_euclid_outreach_fdw
credit
char
description
char
euclid_outreach_oid
meta.oid
int
fov_size
double
id
meta.id;meta.main
char
large_url
char
pixel_size
char
priority
int
rotation
double
stc_s
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
char
primary
title
char
primary
images.mv_hst_outreach_ext_fdw
credit
char
description
char
fov_size
double
hst_outreach_oid
meta.oid
int
id
meta.id;meta.main
char
large_url
char
pixel_size
char
priority
int
rotation
double
stc_s
pos.outline
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
char
primary
title
char
primary
images.mv_hst_outreach_fdw
credit
char
description
char
fov_size
double
hst_outreach_oid
meta.oid
int
id
meta.id;meta.main
char
large_url
char
pixel_size
char
priority
int
rotation
double
stc_s
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
char
primary
title
char
primary
images.mv_webb_outreach_ext_fdw
credit
null
char
description
null
char
fov_size
degrees
null
double
id
meta.id;meta.main
char
large_url
null
char
pixel_size
null
char
priority
null
int
rotation
degrees
null
double
stc_s
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
null
char
webb_outreach_oid
meta.oid
int
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
null
char
primary
title
null
char
primary
images.mv_webb_outreach_fdw
credit
char
description
char
fov_size
degrees
double
id
meta.id;meta.main
char
large_url
char
pixel_size
char
priority
int
rotation
degrees
double
stc_s
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
char
webb_outreach_oid
meta.oid
int
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
char
primary
title
char
primary
images.webb_outreach
credit
char
description
char
fov_size
double
id
meta.id;meta.main
char
large_url
char
pixel_size
char
priority
int
rotation
double
stc_s
obscore:Char.SpatialAxis.Coverage.Support.Area
char
tiles_url
char
webb_outreach_oid
meta.oid
int
fov
pos.outline;meta.pgsphere
char
npix
long
ra_deg
degrees
pos.eq.ra;meta.main
double
dec_deg
degrees
pos.eq.dec;meta.main
double
object_name
char
primary
title
char
primary
layouts
layouts.layout_keys
id
int
is_shown
boolean
"key"
char
observations
observations.mv_akari_irc_fdw
akari_irc_oid
int
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
instrument
The Akari instrument
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
archive_url
The URL to open the archive for the specfic observation
meta.ref.url
char
obs_id
Akari observation identifier
meta.id;meta.main
char
primary
target_name
Target name
char
primary
ra_deg
Right ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C25
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_chandra_obs_photo_fdw
access_estsize
Estimated size of dataset in kB
kB
phys.size;meta.file
obscore:Access.Size
int
access_format
File content format
meta.id;class
obscore:Access.Format
char
calib_level
Calibration level
meta.id;class
obscore:Obs.calibLevel
int
chandra_obs_photo_oid
meta.id
long
dataproduct_subtype
Data product specific type
meta.id;class
obscore:Char.dataProductSubtype
char
dataproduct_type
Logical data product type
meta.id;class
obscore:Obs.dataProductType
char
data_rights
Data rights
meta.code
obscore:Curation.Rights
char
em_calib_status
Type of spectral coord calibration
meta.code.qual
obscore:Char.SpatialAxis.calibStatus
char
em_max
Stop in spectral coordinates
m
em.wl;stat.max
obscore:Char.SpectralAxis.Coverage.Bounds.Limits.Interval.HiLim
double
em_min
Start in spectral coordinates
m
em.wl;stat.min
obscore:Char.SpectralAxis.Coverage.Bounds.Limits.Interval.LoLim
double
em_res_power
Spectral resolving power
m
spec.resolution
obscore:Char.SpectralAxis.Resolution.resolpower.refval
double
em_res_power_max
Resolving power max value on spectral axis
m
spect.resolution;stat.min
obscore:Char.SpatialAxis.Resolution.resolPower.HiLim
double
em_res_power_min
Resolving power min value on spectral axis
m
spect.resolution;stat.min
obscore:Char.SpatialAxis.Resolution.resolPower.LoLim
double
em_ucd
Nature of the spectral axis
meta.ucd
obscore:Char.SpatialAxis.ucd
char
em_unit
Units along the spectral axis
meta.unit
obscore:Char.SpatialAxis.unit
char
facility_name
Name of the instrument used for this observation
meta.id;instr.tel
obscore:Provenance.ObsConfig.Facility.name
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
obs_collection
Name of the data collection
meta.id
obscore:DataID.Collection
char
obs_creation_date
Date when the dataset was created
time;meta.dataset
obscore:DataID.Date
char
obs_creator_did
IVOA dataset identifier given by the creator
meta.id
obscore:DataID.CreatorDID
char
obs_creator_name
Name of the creator of the data
meta.id;creator
obscore:DataID.Creator
char
obs_publisher_did
Dataset identifier given by the publisher
meta.ref.url;meta.curation
obscore:Curation.PublisherDID
char
obs_release_date
Observation release date (ISO 8601)
time.release
obscore:Curation.releaseDate
char
obs_title
Brief description of dataset in free format
meta.title;obs
obscore:DataID.Title
char
o_calib_status
Level of calibration for the observable coord
stat.error;phot.flux
obscore:Char.ObservableAxis.Accuracy.StatError.Refval.value
char
o_stat_error_type
Error
meta.stat.error
char
o_ucd
UCD of observable (e.g. phot.flux.density)
meta.ucd
obscore:Char.ObservableAxis.ucd
char
o_unit
Units used for the observable values
meta.unit
obscore:Char.ObservableAxis.unit
char
pol_states
List of polarization states or NULL if not applicable
meta.code;phys.polarization
obscore:Char.PolarisationAxis.stateList
char
proposal_id
Identifier of proposal to which observation belongs
meta.id;obs.proposal
obscore:Provenance.proposalID
char
publisher_id
IVOA-ID for the Publisher
meta.ref.url;meta.curation
obscore:Curation.PublisherID
char
s_calib_status
Type of calibration along the spatial axis
meta.code.qual
obscore:Char.SpatialAxis.calibStatus
char
s_fov
Diameter (bounds) of the covered region
deg
phys.angSize;instr.fov
obscore:Char.SpatialAxis.Coverage.Bounds.Extent.diameter
double
s_region
Region covered as specified in STC or ADQL
deg
phys.area;obs
obscore:Char.SpatialAxis.Coverage.Support.Area
char
s_resolution
Spatial resolution of data as FWHM
arcsec
pos.angResolution
obscore:Char.SpatialAxis.Resolution.refval.cresolution
double
s_resolution_max
Resolution max value on spectral axis
arcsec
pos.angResolution;stat_max
obscore:Char.SpatialAxis.Resolution.Bounds.Limits.Interval.HiLim
double
s_resolution_min
Resolution min value on spectral axis (FHWM of PSF)
arcsec
pos.angResolution;stat_min
obscore:Char.SpatialAxis.Resolution.Bounds.Limits.Interval.LoLim
double
s_stat_error
Astrometric precision along the spatial axis
arcsec
stat.error;pos.eq
obscore:Char.SpatialAxis.Accuracy.statError.refval.value
double
target_class
Class of the target object as in SSA
src.class
obscore:Target.class
char
t_calib_status
Type of time coord calibration
meta.code.qual
obscore:Char.TimeAxis.calibStatus
char
t_max
End time in MJD
d
obscore:Char.TimeAxis.Coverage.Bounds.Limits.Interval.StopTime
double
t_resolution
Temporal resolution FWHM
s
time.resolution
obscore:Char.TimeAxis.Resolution.Refval
double
t_stat_error
Time coord statistical error
arcsec
stat.error;time
obscore:Char.TimeAxis.Accuracy.StatError.Refval.value
double
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
access_url
URL used to access (download) dataset
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
obs_id
Observation ID
meta.id;meta.main
obscore:DataID.Creatordid
char
primary
instrument_name
The Chandra instrument
meta.id;instr
obscore:Provenance.ObsConfig.Instrument.name
char
primary
target_name
Target name
meta.id;src
obscore:Target.Name
char
primary
s_ra
Central right ascension, ICRS
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
s_dec
Central declination, ICRS
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C3
double
primary
t_min
Start time in MJD
d
obscore:Char.TimeAxis.Coverage.Bounds.Limits.Interval.StartTime
double
primary
t_exptime
Total exposure time
s
time.duration;obs.exposure
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_chandra_obs_spectra_fdw
access_format
File content format
meta.id;class
obscore:Access.Format
char
calib_level
Calibration level
meta.id;class
obscore:Obs.calibLevel
int
chandra_obs_spectra_oid
meta.id
long
dataproduct_subtype
Data product specific type
meta.id;class
obscore:Char.dataProductSubtype
char
dataproduct_type
Logical data product type
meta.id;class
obscore:Obs.dataProductType
char
data_rights
Data rights
meta.code
obscore:Curation.Rights
char
em_calib_status
Type of spectral coord calibration
meta.code.qual
obscore:Char.SpatialAxis.calibStatus
char
em_max
Stop in spectral coordinates
m
em.wl;stat.max
obscore:Char.SpectralAxis.Coverage.Bounds.Limits.Interval.HiLim
double
em_min
Start in spectral coordinates
m
em.wl;stat.min
obscore:Char.SpectralAxis.Coverage.Bounds.Limits.Interval.LoLim
double
em_res_power
Spectral resolving power
m
spec.resolution
obscore:Char.SpectralAxis.Resolution.resolpower.refval
double
em_res_power_max
Resolving power max value on spectral axis
m
spect.resolution;stat.min
obscore:Char.SpatialAxis.Resolution.resolPower.HiLim
double
em_res_power_min
Resolving power min value on spectral axis
m
spect.resolution;stat.min
obscore:Char.SpatialAxis.Resolution.resolPower.LoLim
double
em_ucd
Nature of the spectral axis
meta.ucd
obscore:Char.SpatialAxis.ucd
char
em_unit
Units along the spectral axis
meta.unit
obscore:Char.SpatialAxis.unit
char
facility_name
Name of the instrument used for this observation
meta.id;instr.tel
obscore:Provenance.ObsConfig.Facility.name
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
obs_collection
Name of the data collection
meta.id
obscore:DataID.Collection
char
obs_creation_date
Date when the dataset was created
time;meta.dataset
obscore:DataID.Date
char
obs_creator_did
IVOA dataset identifier given by the creator
meta.id
obscore:DataID.CreatorDID
char
obs_creator_name
Name of the creator of the data
meta.id;creator
obscore:DataID.Creator
char
obs_publisher_did
Dataset identifier given by the publisher
meta.ref.url;meta.curation
obscore:Curation.PublisherDID
char
obs_release_date
Observation release date (ISO 8601)
time.release
obscore:Curation.releaseDate
char
obs_title
Brief description of dataset in free format
meta.title;obs
obscore:DataID.Title
char
o_calib_status
Level of calibration for the observable coord
stat.error;phot.flux
obscore:Char.ObservableAxis.Accuracy.StatError.Refval.value
char
o_stat_error_type
Error
meta.stat.error
char
o_ucd
UCD of observable (e.g. phot.flux.density)
meta.ucd
obscore:Char.ObservableAxis.ucd
char
o_unit
Units used for the observable values
meta.unit
obscore:Char.ObservableAxis.unit
char
pol_states
List of polarization states or NULL if not applicable
meta.code;phys.polarization
obscore:Char.PolarisationAxis.stateList
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
proposal_id
Identifier of proposal to which observation belongs
meta.id;obs.proposal
obscore:Provenance.proposalID
char
publisher_id
IVOA-ID for the Publisher
meta.ref.url;meta.curation
obscore:Curation.PublisherID
char
s_calib_status
Type of calibration along the spatial axis
meta.code.qual
obscore:Char.SpatialAxis.calibStatus
char
s_fov
Diameter (bounds) of the covered region
deg
phys.angSize;instr.fov
obscore:Char.SpatialAxis.Coverage.Bounds.Extent.diameter
double
s_region
Region covered as specified in STC or ADQL
deg
phys.area;obs
obscore:Char.SpatialAxis.Coverage.Support.Area
char
s_resolution
Spatial resolution of data as FWHM
arcsec
pos.angResolution
obscore:Char.SpatialAxis.Resolution.refval.cresolution
double
s_resolution_max
Resolution max value on spectral axis
arcsec
pos.angResolution;stat_max
obscore:Char.SpatialAxis.Resolution.Bounds.Limits.Interval.HiLim
double
s_resolution_min
Resolution min value on spectral axis (FHWM of PSF)
arcsec
pos.angResolution;stat_min
obscore:Char.SpatialAxis.Resolution.Bounds.Limits.Interval.LoLim
double
s_stat_error
Astrometric precision along the spatial axis
arcsec
stat.error;pos.eq
obscore:Char.SpatialAxis.Accuracy.statError.refval.value
double
target_class
Class of the target object as in SSA
src.class
obscore:Target.class
char
t_calib_status
Type of time coord calibration
meta.code.qual
obscore:Char.TimeAxis.calibStatus
char
t_max
End time in MJD
d
obscore:Char.TimeAxis.Coverage.Bounds.Limits.Interval.StopTime
double
t_resolution
Temporal resolution FWHM
s
time.resolution
obscore:Char.TimeAxis.Resolution.Refval
double
t_stat_error
Time coord statistical error
arcsec
stat.error;time
obscore:Char.TimeAxis.Accuracy.StatError.Refval.value
double
access_url
URL used to access (download) dataset
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
obs_id
Observation ID
meta.id;meta.main
obscore:DataID.Creatordid
char
primary
s_ra
Central right ascension, ICRS
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2d.Valu
double
primary
s_dec
Central declination, ICRS
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2d.Valu
double
primary
target_name
Target name
meta.id;src
obscore:Target.Name
char
primary
instrument_name
The Chandra instrument
meta.id;instr
obscore:Provenance.ObsConfig.Instrument.name
char
primary
t_min
Start time in MJD
d
obscore:Char.TimeAxis.Coverage.Bounds.Limits.Interval.StartTime
double
primary
t_exptime
Total exposure time
s
time.duration;obs.exposure
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
access_estsize
Estimated size of dataset in kB
kB
phys.size;meta.file
obscore:Access.Size
int
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_cheops_obs_fdw
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center for nside 256
long
sci_cor_lc_opt_link
The URL to download the Optimal Lightvurve fits file
meta.ref.url;meta.product
char
primary
quality_report_link
The URL to download the Data Reduction Report
meta.ref.url;meta.product
char
primary
targname
Name of target for the observation
char
primary
ra_deg
Right Ascension (J2000)
degrees
pos.eq.ra;meta.main
double
primary
dec_deg
Declination (J2000)
degrees
pos.eq.dec;meta.main
double
primary
mag_g
Brightness of the target in Gaia band
mag
double
primary
mag_chps
Brightness of the target in Cheops band
mag
double
primary
obs_id
Observation ID
meta.id;meta.main
int
primary
v_start_u
Start of observation time in UTC
time.start
char
primary
v_stop_u
End of observation time in UTC
time.end
char
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
cheops_obs_oid
int
observations.mv_efeds_obs_fdw
"area"
double
efeds_obs_oid
null
meta.oid
int
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
prod_url
URL of associated data product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
obsid
Observation ID
meta.id;meta.main;meta.dataset
char
primary
ra_pnt
scheduled pointing direction
deg
pos.eq.ra;meta.main
double
primary
dec_pnt
scheduled pointing direction
deg
pos.eq.dec;meta.main
double
primary
object
Target from proposal
meta.id;src
char
primary
"date-obs"
Start Time (UTC) of first exposure
time.start;obs
char
primary
obs_mode
obsmode: SURVEY or POINTING
obs.param;obs
char
"date-end"
End Time (UTC) of last exposure
time.end;obs
char
primary
emin1
lower boundary energy interval
keV
double
emax1
upper boundary energy interval
keV
double
ra_bary
barycenter of observation footprint
deg
pos.eq.ra;pos.barycenter
double
dec_bary
barycenter of observation footprint
deg
pos.eq.dec;pos.barycenter
double
stcs
Footprint as space-time coordinate string
pos.eq;pos.outline
obscore:Char.SpatialAxis.Coverage.Support.Area
char
fieldid
Observation field identifier
char
texp
combined observation time
s
time.duration;obs.exposure
double
nexp
number of observations
meta.number;obs.exposure
long
observations.mv_euclid_mosaic_product_nisp
fov
pos.outline;meta.pgsphere
double
npix
int
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
dec
Declination of the FPA, in degrees.
deg
pos.eq.dec;meta.main
double
primary
ra
Right ascension of the FPA, in degrees.
deg
pos.eq.ra;meta.main
double
primary
tile_index
long
primary
filter_name
Instrument filter name
char
primary
instrument_name
Name of the instrument [None]
char
primary
file_name
File name of the associated file
meta.id;meta.main
char
primary
observations.mv_euclid_mosaic_product_vis
fov
pos.outline;meta.pgsphere
double
npix
int
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
dec
Declination of the FPA, in degrees.
deg
pos.eq.dec;meta.main
double
primary
ra
Right ascension of the FPA, in degrees.
deg
pos.eq.ra;meta.main
double
primary
tile_index
long
primary
filter_name
Instrument filter name
char
primary
instrument_name
Name of the instrument [None]
char
primary
file_name
File name of the associated file
meta.id;meta.main
char
primary
observations.mv_ida_data_fdw
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C11
double
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
instrument
Name of the instrument used for this observation
obscore:Provenance.ObsConfig.Instrument.name
char
observation_id
Observation identifier for the ISO observations
obscore:DataID.Creatordid
char
observation_oid
Observation internal identifier
int
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
ra_deg
Time-averaged flux in the 20-40 keV band. Appropriate conversion factors are: (20-40keV) 10mCrab=7.57e-11erg/cm2/s=1.71e-3ph/cm2/s.
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C13
double
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_iso_spectra_fdw
data_product_type
Data product type: lsan: ; lsp : ; lsph : ; psp/P40 : ; psph : ; ssph : ; swaa : SWS Auto-Analysis Results;
obscore:Obs.dataProductType
char
dec_deg
Central declination of observations given in the J2000 equatorial system.
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C12
double
end_time_jd
The end time of the observation in Julian Days
d
float
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
fov_col1
fov_col1 and fov_col2 give the maximum field of view of the observation. For rectangular apertures, the sizes are given as parallel to the spacecraft Z and Y axis, respectively. For circular apertures, the diameter is given. For rasters, the field of view is calculated from the apertures and the raster parameters MxN respectively (number of points in a scanline X number of scanlines). If the resulting map presents gaps, the string "(sparse)" is attached. For observations performed in tracking mode (such as on Solar System Objects), the object-centered field-of-view is given (however the whole tracking raster area on the sky is taken into account in the search by position query).
arcsec
double
fov_col2
fov_col1 and fov_col2 give the maximum field of view of the observation. For rectangular apertures, the sizes are given as parallel to the spacecraft Z and Y axis, respectively. For circular apertures, the diameter is given. For rasters, the field of view is calculated from the apertures and the raster parameters MxN respectively (number of points in a scanline X number of scanlines). If the resulting map presents gaps, the string "(sparse)" is attached. For observations performed in tracking mode (such as on Solar System Objects), the object-centered field-of-view is given (however the whole tracking raster area on the sky is taken into account in the search by position query).
arcsec
double
is_validated
The OLP processing software that produced the current Archive products has been declared scientifically validated by the relevant instrument teams.
boolean
observation_id
Observation identifier for the ISO observations
meta.id;meta.main
obscore:DataID.Creatordid
char
observation_id_aux
The TDT number of the observation. This number uniquely identifies an ISO observation.
char
observing_mode
The ISO observing modes: L01 : medium-resolution grating wavelength range spectrum; L02 : grating line spectra; L03 : Fabry-Pérot wavelength range spectrum; L04 : Fabry-Pérot line spectra; P40 : spectrophotometry with PHT-S; S01 : low-resolution full grating scan; S02 : grating line profile scan; S06 : grating scan; S07 : combined Fabry-Pérot line Scan and SW grating scan
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
ra_deg
Central right ascension of observations given in the J2000 equatorial system.
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C12
double
ra_hours
Right ascencsion in decimal hours
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
roll_angle
Reference instrument J2000 role angle
deg
char
start_time_jd
The start time of the observation in Julian Days
d
float
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
stc_s_circle
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
target_name
Target name as given by proposer
obscore:Target.Name
char
observations.mv_iue_spectra_fdw
class
The IUE Object Classification code for the target
char
dec1950
The Homogeneous Declination of the object for equinox B1950.
char
decb1950
The Homogeneous Declination of the object for equinox B1950 in degrees.
deg
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C27
double
decb1950_j2000
deg
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C28
double
dec_target
The target Declination for equinox B1950 as provided by the Guest Observer.
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C26
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
object
The Homogeneous Object Identifier (HOI) for the target. This field has been defined only for output purposes. It is one of the names of the object given by SIMBAD, or following the IAU Minor Planet Center recommendations in the case of comets and asteroids.
char
oid
long
posangle
The position angle of the large aperture during the observation.
deg
double
ra1950
The Homogeneous Right Ascension of the object for equinox B1950.
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C4
char
rab1950
The Homogeneous Right Ascension of the object for equinox B1950 in degrees.
deg
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C5
double
rab1950_j2000
deg
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C6
double
ra_target
The target Right Ascension for equinox B1950 as provided by the Guest Observer.
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C3
char
stc_s_circle
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Observation identifier for the IUE observations
obscore:DataID.Creatordid
char
primary
ra_deg
The Homogeneous Declination of the object for equinox J2000 in degrees.
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C19
double
primary
dec_deg
The Homogeneous Right Ascension of the object for equinox J2000 in degrees.
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C5
double
primary
target_name
The target name as provided by the Guest Observer.
obscore:Target.Name
char
primary
aperture
The aperture used for the exposure: Large: large aperture, 10x20 arcsec oval; Small: small aperture, 3 arcsec diameter circle; N/A: not applicable (e.g. NULL and flat field images).
char
primary
disp
The dispersion mode of the observation: Low : low resolution, ~6Å; High : high resolution, ~0.2Å; N/A : not applicable (e.g. NULL and flat field images).
char
primary
start_time
The U.T. date and time of the start of the exposure
time.start
char
primary
duration
The effective exposure time in seconds, i.e. the commanded exposure time corrected for camera rise time and exposure quantization, and for aperture length and trail rate quantization for trailed exposures.
s
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
filename
Filename(camera)(number)(disp)(aper).FITS
char
observations.mv_nida_images_fdw
archive_link
meta.ref.url
char
primary
end_time
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
nida_images_oid
long
postcard_url
meta.ref.url;meta.preview
char
primary
product_url
obscore:Access.Reference
char
primary
stc_s
char
wavelengths
char
identifier
meta.id;meta.main
char
primary
ra
degrees
pos.eq.ra;meta.main
double
primary
dec
deg
pos.eq.dec;meta.main
double
primary
target
char
primary
object_type
char
primary
start_time
time.start
char
primary
instrument
char
primary
scientific_flag
char
primary
min_wavelength
double
primary
max_wavelength
double
primary
observations.mv_spitzer_irac_fdw
end_time_mjd
Observation End Time
MJD
double
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
oid
long
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
start_time_mjd
Observation Start Time
MJD
double
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
obs_id
meta.id;meta.main
char
primary
instrument
Instrument
char
primary
ra_deg
Right ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C22
double
primary
start_time
Observation Start Time
time
time.start
char
primary
stop_time
Observation Stop Time
time
char
primary
duration
Observation duration
s
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_suzaku_data_fdw
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
observation_oid
Observation internal identifier
int
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Observation ID
meta.id;meta.main
char
primary
instrument
Suzaku instrument
char
primary
ra_deg
Right Ascension (Pointing Position)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C3
double
primary
dec_deg
Declination (Pointing Position)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C21
double
primary
target
Designation of the Pointed Source
char
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_corot_astero_fdw
datalink
Corot Datalink to high level products
meta.dataset;meta.ref.url
char
indexed
corot
[1/21960] (corotid) ID of the CoRoT target
meta.id;meta.main
short
indexed
raj2000
(alpha) Right ascension of star, J2000
deg
pos.eq.ra;meta.main
double
dej2000
(delta) Declination, J2000 (degrees)
deg
pos.eq.dec;meta.main
double
filedate
(crea_dat) File generation date
s
time.epoch;meta.file
int
pv
(pipe_ver) Pipeline process version
meta.software
char
n2v
(n2_ver) Version of N2 data
meta.software
char
date1
(startdat) UT date of first measurement
s
time.epoch
int
date2
(end_date) UT date of last measurment
s
time.epoch
int
spt
? (spectral_type) Spectral type, from EXODAT
src.spType
char
run
[SLIRca0-9] (run_code) (G1)
meta.id;obs
char
ccd
? (hlfccdid) reference of the half CCD from which the product originates e.g. 'E1R' for Right CCD#1 of Exoplanet channel
obs.field
char
magnit_v
? (magnit_v) Visual magnitude of the target
mag
phot.mag;em.opt.V
double
"(b-v)"
? (mag_diff) Color index (B-V)
mag
phot.color
double
npix
Healpix pixel of the center of the observation for nside 256
long
recno
Record number assigned by the VizieR team. Should Not be used for identification.
meta.record
int
"size"
? (filesize) [17280,32921280] bytes in file
Mbyte
meta.note
double
star
Name of the star observed
meta.id
char
absm_v
? (absm_v) Star absolute magnitude in V
mag
meta.id
double
teff
? (teff) Star effective temperature
K
phys.temperature.effective
int
logg
? (gravity) Star gravity (log scale)
log(cm.s**-2)
meta.id
double
"[fe/h]"
? (metal) Star metallicity (log scale)
log(Sun)
phys.abund.Z
double
lcmean
? (lc_mean) light curve mean intensity
ct/s
phot.mag;stat.mean
double
lcrms
? (lc_rms) light curve rms
ct/s
src.var.amplitude
double
assocdata
Associated data file type
char
filename
(filename) Name of file with time series
meta.id;time.epoch;meta.file
char
s_region
Region covered as specified in STC or ADQL
deg
phys.area;obs
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_corot_exo_fdw
datalink
Corot Datalink to high level products
meta.dataset;meta.ref.url
char
indexed
raj2000
(alpha) Right ascension of star, J2000
deg
pos.eq.ra;meta.main
double
dej2000
(delta) Declination, J2000 (degrees)
deg
pos.eq.dec;meta.main
double
pv
(pipe_ver) Pipeline process version
meta.software
char
n2v
(n2_ver) Version of N2 data
meta.software
char
col
[01] 0 = monochrome results, 1 = 3-channels
meta.note
char
date1
(startdat) UT date of first measurement
s
time.epoch
int
date2
(end_date) UT date of last measurement
s
time.epoch
int
corot
[100396342/739016552] (corotid) ID of the CoRoT target
meta.id;meta.main
int
indexed
spt
? (spectral_type) Spectral type, from EXODAT
src.spType
char
"e(b-v)"
? (E(B-V)) E(B-V) colour excess, from EXODAT
mag
phot.color.excess
double
run
[SLIRca0-9] (run_code) (G1)
meta.id;obs
char
ccd
(hlfccdid) reference of the half CCD from which the product originates e.g. E1R for Right CCD#1 of Exoplanet channel
obs.field
char
wid
? (win_id) Window identification
meta.id
short
mag
? (magnitud) Magnitude of the target
mag
phot.mag;em.opt
double
recno
Record number assigned by the VizieR team. Should Not be used for identification.
meta.record
int
filedate
(crea_dat) File generation date
s
time.epoch
int
contf
[0,1]? (contfact) contamination factor
stat.fit.param
double
"exp"
[-1,512]? (exptime) Exposure time
s
time.duration;obs.exposure
short
bmag
? (magnit_b) Star magnitude B
mag
phot.mag;em.opt.B
double
vmag
? (magnit_v) Star magnitude V
mag
phot.mag;em.opt.V
double
rmag
? (magnit_r) Star magnitude R
mag
phot.mag;em.opt.R
double
imag
? (magnit_i) Star magnitude I
mag
phot.mag;em.opt.I
double
tcol
[-1,41510]? (coltemp) Color temperature
K
phys.temperature
int
lcmean
? (lc_mean) light curve mean
ct/s
phot.mag;stat.mean
double
lcrms
? (lc_rms) light curve rms
ct/s
src.var.amplitude
double
nh
(nbhotpix) Number of hot pixels
pix
meta.number
short
s_region
Region covered as specified in STC or ADQL
deg
phys.area;obs
obscore:Char.SpatialAxis.Coverage.Support.Area
char
bmean
? (lc_rms_b) light curve mean B
ct/s
phot.mag;stat.mean
double
gmean
? (lc_rms_g) light curve mean G
ct/s
phot.mag;stat.mean
double
rmean
? (lc_rms_r) light curve mean R
ct/s
phot.mag;stat.mean
double
wmean
? (lc_rms_r) light curve mean white light
ct/s
phot.mag;stat.mean
double
brms
? (lc_rms_b) light curve rms B
ct/s
src.var.amplitude
double
grms
? (lc_rms_g) light curve rms G
ct/s
src.var.amplitude
double
rrms
? (lc_rms_r) light curve rms R
ct/s
src.var.amplitude
double
wrms
? (lc_rms_r) light curve rms white light
ct/s
src.var.amplitude
double
"size"
? Size of file (bytes)
Mbyte
meta.note
double
assocdata
Associated data file type
char
filename
(filename) Name of file with time series
meta.id;time.epoch;meta.file
char
w_file
Name of associated WINDESCRIPTOR file
meta.id;meta.file
char
npix
Healpix pixel of the center of the observation for nside 256
long
observations.mv_v_esasky_xmm_om_optical_fdw
end_utc
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
position_angle
double
proprietary_end_date
char
xmm_om_optical_oid
long
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
The XMM-Newton observation identification
obscore:DataID.Creatordid
char
primary
instrument
Instrument
obscore:Provenance.ObsConfig.Instrument.name
char
primary
observation_oid
Observation internal identifier
int
filter
Filter
char
primary
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C6
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C18
double
primary
target
char
primary
start_utc
time.start
char
primary
duration
Total exposure time of observation
s
obscore:Char.TimeAxis.Coverage.Support.Extent
long
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_esasky_xmm_om_uv_fdw
end_utc
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
position_angle
double
proprietary_end_date
char
xmm_om_uv_oid
long
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
The XMM-Newton observation identification
obscore:DataID.Creatordid
char
primary
instrument
Instrument
obscore:Provenance.ObsConfig.Instrument.name
char
primary
observation_oid
Observation internal identifier
int
filter
Filter
char
primary
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C7
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C17
double
primary
target
char
primary
start_utc
time.start
char
primary
duration
Total exposure time of observation
s
obscore:Char.TimeAxis.Coverage.Support.Extent
long
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_jwst_obs_fdw
access_estsize
long
access_format
char
access_url
char
calib_level
int
core_id
char
dataproduct_type
char
datarelease
char
em_max
double
em_min
double
em_res_power
double
em_ucd
char
em_xel
long
facility_name
char
fov
pos.outline;meta.pgsphere
char
instrument_name
char
lastmodified
char
metarelease
char
obs_collection
char
obs_id
meta.id;meta.main
char
obs_publisher_did
char
obs_release_date
char
o_ucd
char
planeid
char
pol_states
char
pol_xel
int
position_bounds_area
double
position_bounds_center
char
position_bounds_spoly
char
s_dec
pos.eq.dec;meta.main
double
s_fov
double
s_ra
pos.eq.ra;meta.main
double
s_region
char
s_resolution
double
s_xel1
long
s_xel2
long
target_name
char
t_exptime
double
t_max
double
t_min
double
t_resolution
double
t_xel
long
v_jwst_obs_oid
int
observations.mv_v_nida_spectra_fdw
archive_url
meta.ref.url
char
end_time
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
max_wavelength
double
min_wavelength
double
nida_spectra_oid
meta.oid
long
object_type
char
scientific_flag
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
identifier
meta.id;meta.main
char
primary
ra_deg
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
dec_deg
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C23
double
primary
target
char
primary
start_time
time.start
char
primary
instrument
char
primary
wavelengths
char
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_obscore_isla_fdw_fdw
calib_level
int
dataproduct_type
char
em_max
double
em_min
double
npix
Healpix pixel of the center of the observation for nside 256
long
obs_collection
char
obs_oid
long
s_fov
double
access_url
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
obs_id
meta.id;meta.main
char
primary
instrument_name
char
primary
s_ra
pos.eq.ra;meta.main
double
primary
s_dec
pos.eq.dec;meta.main
double
primary
t_min
double
primary
t_max
double
primary
t_exptime
double
primary
access_estsize
B
phys.size;meta.file
obscore:Access.Size
long
primary
target_name
char
primary
observations.mv_v_v_alma_obs_fdw
dataproduct_type
char
em_max
Stop in spectral coordinates
m
obscore:Char.SpectralAxis.Coverage.Bounds.Limits.Interval.HiLim
double
em_min
Start in spectral coordinates
m
obscore:Char.SpectralAxis.Coverage.Bounds.Limits.Interval.LoLim
double
em_res_power
Spectral resolving power
m
obscore:Char.SpectralAxis.Resolution.resolpower.refval
double
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
frequency_support
char
obs_id
char
obs_publisher_did
char
obs_release_date
char
pol_states
char
scan_intent
char
science_keyword
char
s_region
Region bounded by observation
deg
char
t_max
End time of observation (MJD)
d
double
v_alma_obs_oid
int
access_url
URL. to download the data
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Dataset identifier
meta.id;meta.main
char
primary
s_ra
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
s_dec
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C4
double
primary
s_fov
Size of the region covered (~diameter of minimum bounding circle)
deg
obscore:Char.SpatialAxis.Coverage.Bounds.Extent.diameter
double
target_name
Name of intended target
char
primary
t_min
Start time of observation (MJD)
d
double
primary
t_exptime
Exposure time of observation
s
double
primary
band_list
Space delimited list of bands
char
primary
freq_min
Minimum frequency of observation
GHz
double
primary
freq_max
Maximum frequency of observation
GHz
double
primary
scientific_category
Scientific category
char
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_esasky_jwst_images_fdw_fdw
JWST Observations (Near-Infrared)
collection
Name of the data collection
meta.id
char
data_product_type
Data product type
char
data_release
Date the data for a plane is public (UTC)
caom2:Plane.dataRelease
char
detector
Name of the detector defined in instrument_keywords
char
end_time
Stop time in MJD
d
time.end;obs.exposure
Char.TimeAxis.Coverage.Bounds.Limits.StopTime
char
energy_bounds_lower
Start in spectral coordinates
m
em.wl;stat.min
Char.SpectralAxis.Coverage.Bounds.Limits.LoLimit
double
energy_bounds_upper
Stop in spectral coordinates
m
em.wl;stat.max
Char.SpectralAxis.Coverage.Bounds.Limits.HiLimit
double
energy_bounds_width
Width of the energy bounds
m
double
fov
Diameter (bounds) of the covered region
deg
pos.outline;meta.pgsphere
Char.SpatialAxis.Coverage.Bounds.Extent.diameter
char
intent
Intended purpose of data (one of: science, calibration)
char
members
Observations used to generate this on
int
npix
Healpix pixel of the center of the observation for nside 256
long
obsid
Foreign key
char
plane_id
Unique plane identifier
caom2:Plane.id
char
proposal_keywords
Proposal keywords (separated by |)
char
proposal_pi
Proposal Principal Investigator
char
subarray
SUBARRAY field extracted from instrument_keywords
char
target_category
TARGETCATEGORY parameter extracted from target_keywords
char
target_keywords
Target keywords (separated by |)
char
target_moving
Flag for moving target
boolean
template
TEMPLATE parameter extracted from instrument_keywords
char
wave_central
Central wavelength in spectral coordinates
double
product_url
URL used to access (download) the dataset
meta.ref.url
obscore:Access.Reference
char
primary
postcard_url
URL used to access (download) the postcard
meta.ref.url;meta.preview
char
primary
observation_id
Observation ID
meta.id;meta.main
DataID.observationID
char
primary
target_name
Astronomical object observed, if any
meta.id;src
Target.name
char
primary
ra_deg
Central right ascension, ICRS
deg
pos.eq.ra;meta.main
Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
dec_deg
Central declination, ICRS
deg
pos.eq.dec;meta.main
Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C2
double
primary
instrument
Name of the instrument used for this observation
meta.id;instr
Provenance.ObsConfig.Instrument.name
char
primary
observing_mode
Observing Mode extracted from EXP_KEY keyword
char
primary
proposal_id
Collection-specific unique proposal identifier
char
primary
calibrationlevel
Calibration level {0, 1, 2, 3, 4}
int
primary
start_time
Start time in MJD
d
time.start;obs.exposure
Char.TimeAxis.Coverage.Bounds.Limits.StartTime
char
primary
duration
Total exposure time
s
time.duration;obs.exposure
Char.TimeAxis.Coverage.Support.Extent
double
primary
filter
Collection-specific name for energy band (e.g. filter name)
char
primary
stc_s
Sky region covered by the data product(expressed in ICRS frame)
pos.outline;obs.field
Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_esasky_jwst_images_miri_fdw_fdw
JWST Observations (Mid-Infrared)
collection
Name of the data collection
meta.id
char
data_product_type
Data product type
char
data_release
Date the data for a plane is public (UTC)
caom2:Plane.dataRelease
char
detector
Name of the detector defined in instrument_keywords
char
end_time
Stop time in MJD
d
time.end;obs.exposure
Char.TimeAxis.Coverage.Bounds.Limits.StopTime
char
energy_bounds_lower
Start in spectral coordinates
m
em.wl;stat.min
Char.SpectralAxis.Coverage.Bounds.Limits.LoLimit
double
energy_bounds_upper
Stop in spectral coordinates
m
em.wl;stat.max
Char.SpectralAxis.Coverage.Bounds.Limits.HiLimit
double
energy_bounds_width
Width of the energy bounds
m
double
fov
Diameter (bounds) of the covered region
deg
pos.outline;meta.pgsphere
Char.SpatialAxis.Coverage.Bounds.Extent.diameter
char
intent
Intended purpose of data (one of: science, calibration)
char
members
Observations used to generate this on
int
npix
Healpix pixel of the center of the observation for nside 256
long
obsid
Foreign key
char
plane_id
Unique plane identifier
caom2:Plane.id
char
proposal_keywords
Proposal keywords (separated by |)
char
proposal_pi
Proposal Principal Investigator
char
subarray
SUBARRAY field extracted from instrument_keywords
char
target_category
TARGETCATEGORY parameter extracted from target_keywords
char
target_keywords
Target keywords (separated by |)
char
target_moving
Flag for moving target
boolean
template
TEMPLATE parameter extracted from instrument_keywords
char
wave_central
Central wavelength in spectral coordinates
double
product_url
URL used to access (download) the dataset
meta.ref.url
obscore:Access.Reference
char
primary
postcard_url
URL used to access (download) the postcard
meta.ref.url;meta.preview
char
primary
observation_id
Observation ID
meta.id;meta.main
DataID.observationID
char
primary
target_name
Astronomical object observed, if any
meta.id;src
Target.name
char
primary
ra_deg
Central right ascension, ICRS
deg
pos.eq.ra;meta.main
Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
dec_deg
Central declination, ICRS
deg
pos.eq.dec;meta.main
Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C2
double
primary
instrument
Name of the instrument used for this observation
meta.id;instr
Provenance.ObsConfig.Instrument.name
char
primary
observing_mode
Observing Mode extracted from EXP_KEY keyword
char
primary
proposal_id
Collection-specific unique proposal identifier
char
primary
calibrationlevel
Calibration level {0, 1, 2, 3, 4}
int
primary
start_time
Start time in MJD
d
time.start;obs.exposure
Char.TimeAxis.Coverage.Bounds.Limits.StartTime
char
primary
duration
Total exposure time
s
time.duration;obs.exposure
Char.TimeAxis.Coverage.Support.Extent
double
primary
filter
Collection-specific name for energy band (e.g. filter name)
char
primary
stc_s
Sky region covered by the data product(expressed in ICRS frame)
pos.outline;obs.field
Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_esasky_jwst_spectra_fdw_fdw
JWST Spectra (Near-Infrared)
collection
Name of the data collection
meta.id
char
data_product_type
Data product type
char
data_release
Date the data for a plane is public (UTC)
caom2:Plane.dataRelease
char
detector
Name of the detector defined in instrument_keywords
char
end_time
Stop time in MJD
d
time.end;obs.exposure
Char.TimeAxis.Coverage.Bounds.Limits.StopTime
char
energy_bounds_lower
Start in spectral coordinates
m
em.wl;stat.min
Char.SpectralAxis.Coverage.Bounds.Limits.LoLimit
double
energy_bounds_upper
Stop in spectral coordinates
m
em.wl;stat.max
Char.SpectralAxis.Coverage.Bounds.Limits.HiLimit
double
energy_bounds_width
Width of the energy bounds
m
double
fov
Diameter (bounds) of the covered region
deg
pos.outline;meta.pgsphere
Char.SpatialAxis.Coverage.Bounds.Extent.diameter
char
intent
Intended purpose of data (one of: science, calibration)
char
members
Observations used to generate this on
int
npix
Healpix pixel of the center of the observation for nside 256
long
obsid
Foreign key
char
plane_id
Unique plane identifier
caom2:Plane.id
char
proposal_keywords
Proposal keywords (separated by |)
char
proposal_pi
Proposal Principal Investigator
char
subarray
SUBARRAY field extracted from instrument_keywords
char
target_category
TARGETCATEGORY parameter extracted from target_keywords
char
target_keywords
Target keywords (separated by |)
char
target_moving
Flag for moving target
boolean
template
TEMPLATE parameter extracted from instrument_keywords
char
wave_central
Central wavelength in spectral coordinates
double
product_url
URL used to access (download) the dataset
meta.ref.url
obscore:Access.Reference
char
primary
postcard_url
URL used to access (download) the postcard
meta.ref.url;meta.preview
char
primary
observation_id
Observation ID
meta.id;meta.main
DataID.observationID
char
primary
target_name
Astronomical object observed, if any
meta.id;src
Target.name
char
primary
ra_deg
Central right ascension, ICRS
deg
pos.eq.ra;meta.main
Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
dec_deg
Central declination, ICRS
deg
pos.eq.dec;meta.main
Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C2
double
primary
instrument
Name of the instrument used for this observation
meta.id;instr
Provenance.ObsConfig.Instrument.name
char
primary
observing_mode
Observing Mode extracted from EXP_KEY keyword
char
primary
proposal_id
Collection-specific unique proposal identifier
char
primary
calibrationlevel
Calibration level {0, 1, 2, 3, 4}
int
primary
start_time
Start time in MJD
d
time.start;obs.exposure
Char.TimeAxis.Coverage.Bounds.Limits.StartTime
char
primary
duration
Total exposure time
s
time.duration;obs.exposure
Char.TimeAxis.Coverage.Support.Extent
double
primary
filter
Collection-specific name for energy band (e.g. filter name)
char
primary
stc_s
Sky region covered by the data product(expressed in ICRS frame)
pos.outline;obs.field
Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_esasky_jwst_spectra_miri_fdw_fdw
JWST Spectra (Mid-Infrared)
collection
Name of the data collection
meta.id
char
data_product_type
Data product type
char
data_release
Date the data for a plane is public (UTC)
caom2:Plane.dataRelease
char
detector
Name of the detector defined in instrument_keywords
char
end_time
Stop time in MJD
d
time.end;obs.exposure
Char.TimeAxis.Coverage.Bounds.Limits.StopTime
char
energy_bounds_lower
Start in spectral coordinates
m
em.wl;stat.min
Char.SpectralAxis.Coverage.Bounds.Limits.LoLimit
double
energy_bounds_upper
Stop in spectral coordinates
m
em.wl;stat.max
Char.SpectralAxis.Coverage.Bounds.Limits.HiLimit
double
energy_bounds_width
Width of the energy bounds
m
double
fov
Diameter (bounds) of the covered region
deg
pos.outline;meta.pgsphere
Char.SpatialAxis.Coverage.Bounds.Extent.diameter
char
intent
Intended purpose of data (one of: science, calibration)
char
members
Observations used to generate this on
int
npix
Healpix pixel of the center of the observation for nside 256
long
obsid
Foreign key
char
plane_id
Unique plane identifier
caom2:Plane.id
char
proposal_keywords
Proposal keywords (separated by |)
char
proposal_pi
Proposal Principal Investigator
char
subarray
SUBARRAY field extracted from instrument_keywords
char
target_category
TARGETCATEGORY parameter extracted from target_keywords
char
target_keywords
Target keywords (separated by |)
char
target_moving
Flag for moving target
boolean
template
TEMPLATE parameter extracted from instrument_keywords
char
wave_central
Central wavelength in spectral coordinates
double
product_url
URL used to access (download) the dataset
meta.ref.url
obscore:Access.Reference
char
primary
postcard_url
URL used to access (download) the postcard
meta.ref.url;meta.preview
char
primary
observation_id
Observation ID
meta.id;meta.main
DataID.observationID
char
primary
target_name
Astronomical object observed, if any
meta.id;src
Target.name
char
primary
ra_deg
Central right ascension, ICRS
deg
pos.eq.ra;meta.main
Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1
double
primary
dec_deg
Central declination, ICRS
deg
pos.eq.dec;meta.main
Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C2
double
primary
instrument
Name of the instrument used for this observation
meta.id;instr
Provenance.ObsConfig.Instrument.name
char
primary
observing_mode
Observing Mode extracted from EXP_KEY keyword
char
primary
proposal_id
Collection-specific unique proposal identifier
char
primary
calibrationlevel
Calibration level {0, 1, 2, 3, 4}
int
primary
start_time
Start time in MJD
d
time.start;obs.exposure
Char.TimeAxis.Coverage.Bounds.Limits.StartTime
char
primary
duration
Total exposure time
s
time.duration;obs.exposure
Char.TimeAxis.Coverage.Support.Extent
double
primary
filter
Collection-specific name for energy band (e.g. filter name)
char
primary
stc_s
Sky region covered by the data product(expressed in ICRS frame)
pos.outline;obs.field
Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hsa_esasky_photo_fdw_fdw
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
The identifier of a Herschel observation
obscore:DataID.Creatordid
char
primary
observation_oid
Database index number
int
ra_deg
Actual right ascension of pointing
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C10
double
dec_deg
Actual declination of pointing
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C14
double
target_name
The name of the target
obscore:Target.Name
char
primary
instrument
The Herschel instrument
obscore:Provenance.ObsConfig.Instrument.name
char
primary
filter
Filter or filters used
microns
char
primary
start_time
The start date and time of the observation
time.start
char
primary
end_time
The end date and time of the observation
time.end
char
duration
Duration of the observation in seconds
seconds
obscore:Char.TimeAxis.Coverage.Support.Extent
double
observing_mode_name
Name of the Herschel observing mode
char
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hsa_esasky_spectra_fdw_fdw
end_time
The end date and time of the observation
time.end
char
fov
pos.outline;meta.pgsphere
char
instrument_mode
The Herschel instrument mode
char
observation_oid
Database index number
int
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
char
primary
product_url
The URL to download the product
obscore:Access.Reference
char
primary
observation_id
The identifier of a Herschel observation
meta.id;meta.main
char
primary
ra_deg
Actual right ascension of pointing
deg
pos.eq.ra;meta.main
double
primary
dec_deg
Actual declination of pointing
deg
pos.eq.dec;meta.main
double
primary
target_name
The name of the target
char
primary
instrument
The Herschel instrument
char
primary
observing_mode_name
Name of the Herschel observing mode
char
primary
band
Frequency or wavelength band in which the data were taken
char
primary
start_time
The start date and time of the observation
time.start
char
primary
duration
Duration of the observation in seconds
seconds
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hst_mmi_observation_fdw_fdw
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
observation_id
Data set 9 character name. First character indicates instrument; L=COS; I=WFC3; J=ACS; N=NICMOS; O=STIS; U=WFPC2; W=WFPC; X=FOC; Y=FOS; Z=GHRS; F=FGS; V=HSP.
obscore:DataID.Creatordid
char
primary
observation_oid
Observation internal identifier
char
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C14
double
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C10
double
target_name
Observer assigned target name
obscore:Target.Name
char
primary
instrument_name
The HST instrument and channel
obscore:Provenance.ObsConfig.Instrument.name
char
primary
filter
Filter
char
primary
start_time
Observation start time
time
time.start
char
primary
end_time
Observation stop time
time
time.end
char
exposure_duration
Exposure time of observation
s
obscore:Char.TimeAxis.Coverage.Support.Extent
float
collection
The type of Hubble collection. 'HST' is the standard HST archive content; 'HLA' the Hubble Legacy Archive; 'HLSP' High level science product.
obscore:DataID.Collection
char
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hst_mmi_observation_infrared_fdw_fdw
end_time
Observation stop time
time
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
observation_oid
Observation internal identifier
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Data set 9 character name. First character indicates instrument; L=COS; I=WFC3; J=ACS; N=NICMOS; O=STIS; U=WFPC2; W=WFPC; X=FOC; Y=FOS; Z=GHRS; F=FGS; V=HSP.
obscore:DataID.Creatordid
char
primary
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C14
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C10
double
primary
target_name
Observer assigned target name
obscore:Target.Name
char
primary
instrument_name
The HST instrument and channel
obscore:Provenance.ObsConfig.Instrument.name
char
primary
collection
The type of Hubble collection. 'HST' is the standard HST archive content; 'HLA' the Hubble Legacy Archive; 'HLSP' High level science product.
obscore:DataID.Collection
char
primary
obs_type
Type of observation
char
primary
filter
Filter
char
primary
start_time
Observation start time
time
time.start
char
primary
exposure_duration
Exposure time of observation
seconds
obscore:Char.TimeAxis.Coverage.Support.Extent
float
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hst_mmi_observation_optical_fdw_fdw
end_time
Observation stop time
time
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
observation_oid
Observation internal identifier
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Data set 9 character name. First character indicates instrument; L=COS; I=WFC3; J=ACS; N=NICMOS; O=STIS; U=WFPC2; W=WFPC; X=FOC; Y=FOS; Z=GHRS; F=FGS; V=HSP.
obscore:DataID.Creatordid
char
primary
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C15
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C9
double
primary
target_name
Observer assigned target name
obscore:Target.Name
char
primary
instrument_name
The HST instrument and channel
obscore:Provenance.ObsConfig.Instrument.name
char
primary
collection
The type of Hubble collection. 'HST' is the standard HST archive content; 'HLA' the Hubble Legacy Archive; 'HLSP' High level science product.
obscore:DataID.Collection
char
primary
obs_type
char
primary
filter
Filter
char
primary
start_time
Observation start time
time
time.start
char
primary
exposure_duration
Exposure time of observation
seconds
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hst_mmi_observation_uv_fdw_fdw
end_time
Observation stop time
time
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
observation_oid
Observation internal identifier
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Data set 9 character name. First character indicates instrument; L=COS; I=WFC3; J=ACS; N=NICMOS; O=STIS; U=WFPC2; W=WFPC; X=FOC; Y=FOS; Z=GHRS; F=FGS; V=HSP.
obscore:DataID.Creatordid
char
primary
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C16
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C8
double
primary
target_name
Observer assigned target name
obscore:Target.Name
char
primary
instrument_name
The HST instrument and channel
obscore:Provenance.ObsConfig.Instrument.name
char
primary
collection
The type of Hubble collection. 'HST' is the standard HST archive content; 'HLA' the Hubble Legacy Archive; 'HLSP' High level science product.
obscore:DataID.Collection
char
primary
obs_type
char
primary
filter
Filter
char
primary
start_time
Observation start time
time
time.start
char
primary
exposure_duration
Exposure time of observation
seconds
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hst_mmi_spectra_infrared_fdw_fdw
end_time
Observation stop time
time
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
observation_oid
Observation internal identifier
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Data set 9 character name. First character indicates instrument; L=COS; I=WFC3; J=ACS; N=NICMOS; O=STIS; U=WFPC2; W=WFPC; X=FOC; Y=FOS; Z=GHRS; F=FGS; V=HSP.
obscore:DataID.Creatordid
char
primary
target_name
Observer assigned target name
obscore:Target.Name
char
primary
instrument_name
The HST instrument and channel
obscore:Provenance.ObsConfig.Instrument.name
char
primary
obs_type
char
primary
wave_central
Central wavelength
Angstroms
double
primary
filter
Filters/Gratings
char
primary
collection
The type of Hubble collection. 'HST' is the standard HST archive content; 'HLA' the Hubble Legacy Archive; 'HLSP' High level science product.
obscore:DataID.Collection
char
primary
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C17
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C7
double
primary
start_time
Observation start time
time
time.start
char
primary
exposure_duration
Exposure time of observation
seconds
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hst_mmi_spectra_optical_fdw_fdw
collection
The type of Hubble collection. 'HST' is the standard HST archive content; 'HLA' the Hubble Legacy Archive; 'HLSP' High level science product.
obscore:DataID.Collection
char
end_time
Observation stop time
time
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
observation_oid
Observation internal identifier
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Data set 9 character name. First character indicates instrument; L=COS; I=WFC3; J=ACS; N=NICMOS; O=STIS; U=WFPC2; W=WFPC; X=FOC; Y=FOS; Z=GHRS; F=FGS; V=HSP.
obscore:DataID.Creatordid
char
primary
target_name
Observer assigned target name
obscore:Target.Name
char
primary
instrument_name
The HST instrument and channel
obscore:Provenance.ObsConfig.Instrument.name
char
primary
obs_type
char
primary
filter
Filters/Gratings
char
primary
wave_central
Central wavelength
Angstroms
double
primary
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C18
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C6
double
primary
start_time
Observation start time
time
time.start
char
primary
exposure_duration
Exposure time of observation
seconds
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_hst_mmi_spectra_uv_fdw_fdw
collection
The type of Hubble collection. 'HST' is the standard HST archive content; 'HLA' the Hubble Legacy Archive; 'HLSP' High level science product.
obscore:DataID.Collection
char
end_time
Observation stop time
time
time.end
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
observation_oid
Observation internal identifier
char
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
Data set 9 character name. First character indicates instrument; L=COS; I=WFC3; J=ACS; N=NICMOS; O=STIS; U=WFPC2; W=WFPC; X=FOC; Y=FOS; Z=GHRS; F=FGS; V=HSP.
obscore:DataID.Creatordid
char
primary
target_name
Observer assigned target name
obscore:Target.Name
char
primary
instrument_name
The HST instrument and channel
obscore:Provenance.ObsConfig.Instrument.name
char
primary
obs_type
char
primary
filter
Filters/Gratings
char
primary
wave_central
Central wavelength
Angstroms
double
primary
ra_deg
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C9
double
primary
dec_deg
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C15
double
primary
start_time
Observation start time
time
time.start
char
primary
exposure_duration
Exposure time of observation
seconds
obscore:Char.TimeAxis.Coverage.Support.Extent
double
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_xsa_esasky_photo_fdw_fdw
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
position_angle
deg
double
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
The XMM-Newton observation identification
obscore:DataID.Creatordid
char
primary
observation_oid
Observation internal identifier
int
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C4
double
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C20
double
target_name
Target name
obscore:Target.Name
char
primary
instrument
Instrument
obscore:Provenance.ObsConfig.Instrument.name
char
primary
start_time
Observation Start Time
time
time.start
char
primary
end_time
Observation End Time
time
time.end
char
duration
Total exposure time of observation
s
obscore:Char.TimeAxis.Coverage.Support.Extent
long
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.mv_v_v_xsa_spectra_rgs_fdw_fdw
end_utc
Observation End Time
time
char
fov
Internal ESASky column for searching and indexing the footprint with pgsphere
pos.outline;meta.pgsphere
char
npix
Healpix pixel of the center of the observation for nside 256
long
observation_oid
Observation internal identifier
int
position_angle
Position Angle
deg
double
postcard_url
The URL to download the postcard preview
meta.ref.url;meta.preview
obscore:Access.Reference
char
primary
product_url
The URL to download the product
meta.dataset;meta.ref.url
obscore:Access.Reference
char
primary
observation_id
The XMM-Newton observation identification
obscore:DataID.Creatordid
char
primary
ra_deg
Right Ascension (J2000)
deg
pos.eq.ra;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C5
double
primary
dec_deg
Declination (J2000)
deg
pos.eq.dec;meta.main
obscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C19
double
primary
target_name
Target name
obscore:Target.Name
char
primary
instrument
Instrument
obscore:Provenance.ObsConfig.Instrument.name
char
primary
band
Frequency or wavelength band in which the data were taken
char
primary
start_utc
Observation Start Time
time
char
primary
duration
Total exposure time of observation
s
obscore:Char.TimeAxis.Coverage.Support.Extent
long
primary
stc_s
Footprint of the observation in STC string format
obscore:Char.SpatialAxis.Coverage.Support.Area
char
observations.v_mv_v_esasky_xmm_om_fdw
dec_deg
pos.eq.dec;meta.main
double
duration
Total exposure time of observation
s
long
end_utc
char
filter
Filter
char
fov
pos.outline;meta.pgsphere
char
instrument
Instrument
char
npix
Healpix pixel of the center of the observation for nside 256
long
observation_id
The XMM-Newton observation identification
meta.id;meta.main
char
observation_oid
Observation internal identifier
int
position_angle
double
postcard_url
The URL to download the postcard preview
char
product_url
The URL to download the product
char
proprietary_end_date
char
ra_deg
pos.eq.ra;meta.main
double
start_utc
char
stc_s
char
target
char
xmm_om_optical_oid
long
public
public.function_dummy
dummy
int
sso
sso.card_reduction_herschel
epochs
char
positions
char
sso_id
char
sso_name
char
sso_oid
int
sso.card_reduction_hst
epochs
char
positions
char
sso_id
char
sso_name
char
sso_oid
int
sso.card_reduction_xmm
epochs
char
positions
char
sso_id
char
sso_name
char
sso_oid
int
sso.count_metadata
count_column
char
table_name
char
sso.count_table
herschel
int
hst
int
sso_oid
int
xmm
int
xmm_om
int
sso.ssoid
last_update
char
sso_id
char
sso_name
char
sso_oid
int
sso_type
char
sso.xmatch_herschel
dec_deg_1
double
primary
dec_deg_2
double
primary
dist_1
double
primary
dist_2
double
dist_dot_1
double
dist_dot_2
double
elong_1
double
elong_2
double
mu_de_1
double
mu_de_2
double
mu_ra_cos_de_1
double
mu_ra_cos_de_2
double
observation_id
char
observation_oid
int
phase_1
double
phase_2
double
pos1_deg_err
double
primary
pos2_deg_err
double
ra_deg_1
double
primary
ra_deg_2
double
primary
sso_id
char
sso_name
char
primary
sso_oid
int
v_mag_1
double
primary
v_mag_2
double
sso.xmatch_hst
dist_2
double
dist_dot_1
double
dist_dot_2
double
elong_1
double
elong_2
double
mu_de_1
double
mu_de_2
double
mu_ra_cos_de_1
double
mu_ra_cos_de_2
double
observation_id
char
observation_oid
char
phase_1
double
phase_2
double
pos2_deg_err
double
sso_id
char
sso_oid
int
v_mag_2
double
sso_name
char
primary
ra_deg_1
pos.eq.ra
double
primary
dec_deg_1
pos.eq.dec
double
primary
ra_deg_2
double
primary
dec_deg_2
double
primary
pos1_deg_err
double
primary
v_mag_1
double
primary
dist_1
double
primary
sso.xmatch_xmm
dist_2
double
dist_dot_1
double
dist_dot_2
double
elong_1
double
elong_2
double
mu_de_1
double
mu_de_2
double
mu_ra_cos_de_1
double
mu_ra_cos_de_2
double
observation_id
char
observation_oid
int
phase_1
double
phase_2
double
pos2_deg_err
double
sso_id
char
sso_oid
int
v_mag_2
double
sso_name
char
primary
ra_deg_1
pos.eq.ra
double
primary
dec_deg_1
pos.eq.dec
double
primary
ra_deg_2
double
primary
dec_deg_2
double
primary
pos1_deg_err
double
primary
v_mag_1
double
primary
dist_1
double
primary
sso.xmatch_xmm_om
dist_2
double
dist_dot_1
double
dist_dot_2
double
duration
long
elong_1
double
elong_2
double
filter
char
mlim_obs
double
mu_de_1
double
mu_de_2
double
mu_ra_cos_de_1
double
mu_ra_cos_de_2
double
observation_id
char
observation_oid
int
phase_1
double
phase_2
double
pos2_deg_err
double
sso_id
char
sso_oid
int
start_time
char
target_name
char
v_mag_1_corrected
double
v_mag_2
double
xmatch_type
int
sso_name
char
primary
ra_deg_1
pos.eq.ra
double
primary
dec_deg_1
pos.eq.dec
double
primary
ra_deg_2
double
primary
dec_deg_2
double
primary
pos1_deg_err
double
primary
v_mag_1
double
primary
dist_1
double
primary
sso_20190705
sso_20190705.xmatch_herschel_aster
sso_id
sso identifier (astorb database)
char
sso_name
sso name (astorb db)
char
indexed
observation_id
observation identifier
char
indexed
target_name
target name of the observation
char
instrument
instrument of the observation
char
observing_mode_name
Observation Mode
char
start_time
start time of the observation
char
duration
total exposure time of the observation
s
double
filter
filter/band of the observation
char
ra_deg_1
sso expected right ascension (J2000) at the start time of the observation
double
dec_deg_1
sso expected declination (J2000) at the start time of the observation
double
dist_1
expected distance to the sso from the satellite at the start time of the observation
au
double
v_mag_1
sso expected v magnitude at the start time of the observation
double
phase_1
sso expected phase angle at the start time of the observation
deg
double
elong_1
sso expected elongation at the start time of the observation
deg
double
mu_ra_cos_de_1
sso expected proper motion along ra axis at the start time of the observation
arcsec/min
double
mu_de_1
sso expected proper motion along dec axis at the start time of the observation
arcsec/min
double
dist_dot_1
sso expected speed at the start time of the observation
km/s
double
pos1_deg_err
sso positional error at the start time of the observation
deg
double
ra_deg_2
sso positional error at the start time of the observation
double
dec_deg_2
sso expected declination (J2000) at the end time of the observation, end time computed as the start time plus duration of the observation
double
dist_2
expected distance to the sso from the satellite at the end time of the observation, end time computed as the start time plus duration of the observation
au
double
v_mag_2
sso expected magnitude V at the end time of the observation, end time computed as the start time plus duration of the observation
double
phase_2
sso expected phase angle at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
elong_2
sso expected elongation at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
mu_ra_cos_de_2
sso expected proper motion along ra axis at the end time of the observation, end time computed as the start time plus duration of the observation
arcsec/min
double
mu_de_2
sso expected proper motion along dec axis at the end time of the observation, end time computed as the start time plus duration of the observation
arcsec/min
double
dist_dot_2
expected sso distance to the sso from the satellite at the end time of the observation, end time computed as the start time plus duration of the observation
km/s
double
pos2_deg_err
sso expected positional error at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
xmatch_type
type of match (2: inside FoV;1: pos+error radius crossing FoV;3:sso path crossing FoV)
int
flux_70
sso theoretical flux at 70 micron
mJy
double
flux_100
sso theoretical flux at 100 micron
mJy
double
flux_160
sso theoretical flux at 160 micron
mJy
double
flux_250
sso theoretical flux at 250 micron
mJy
double
flux_350
sso theoretical flux at 350 micron
mJy
double
flux_500
sso theoretical flux at 500 micron
mJy
double
is_visible
flag indicating if corresponding detection is above flux sensitivity
boolean
sso_20190705.xmatch_hst_aster
sso_id
sso identifier (astorb database)
char
sso_name
sso name (astorb db)
char
indexed
observation_id
observation identifier
char
indexed
instrument_name
instrument
char
target_name
target name of the observation
char
start_time
start time of the observation
char
exposure_duration
total time duration of the observation
double
ra_deg_1
sso expected right ascension (J2000) at the start time of the observation
double
dec_deg_1
sso expected declination (J2000) at the start time of the observation
double
dist_1
expected distance to the sso from the satellite at the start time of the observation
au
double
v_mag_1
sso expected v magnitude at the start time of the observation
double
phase_1
sso expected phase angle at the start time of the observation
deg
double
elong_1
sso expected elongation at the start time of the observation
deg
double
mu_ra_cos_de_1
sso expected proper motion along ra axis at the start time of the observation
arcsec/min
double
mu_de_1
sso expected proper motion along dec axis at the start time of the observation
arcsec/min
double
dist_dot_1
sso expected speed at the start time of the observation
km/s
double
pos1_deg_err
sso positional error at the start time of the observation
deg
double
ra_deg_2
sso positional error at the start time of the observation
double
dec_deg_2
sso expected declination (J2000) at the end time of the observation, end time computed as the start time plus duration of the observation
double
dist_2
expected distance to the sso from the satellite at the end time of the observation, end time computed as the start time plus duration of the observation
au
double
v_mag_2
sso expected magnitude V at the end time of the observation, end time computed as the start time plus duration of the observation
double
phase_2
sso expected phase angle at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
elong_2
sso expected elongation at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
mu_ra_cos_de_2
sso expected proper motion along ra axis at the end time of the observation, end time computed as the start time plus duration of the observation
arcsec/min
double
mu_de_2
sso expected proper motion along dec axis at the end time of the observation, end time computed as the start time plus duration of the observation
arcsec/min
double
dist_dot_2
expected sso distance to the sso from the satellite at the end time of the observation, end time computed as the start time plus duration of the observation
km/s
double
pos2_deg_err
sso expected positional error at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
xmatch_type
type of match (2: inside FoV;1: pos+error radius crossing FoV;3:sso path crossing FoV)
int
sso_20190705.xmatch_xmm_aster
sso_id
sso identifier (astorb database)
char
sso_name
sso name (astorb db)
char
indexed
observation_id
observation identifier
char
indexed
target_name
target name of the observation
char
filter
filter/band of the observation
char
start_time
start time of the observation
char
duration
total exposure time of the observation
s
long
ra_deg_1
sso expected right ascension (J2000) at the start time of the observation
double
dec_deg_1
sso expected declination (J2000) at the start time of the observation
double
dist_1
expected distance to the sso from the satellite at the start time of the observation
au
double
v_mag_1
sso expected v magnitude at the start time of the observation
double
phase_1
sso expected phase angle at the start time of the observation
deg
double
elong_1
sso expected elongation at the start time of the observation
deg
double
mu_ra_cos_de_1
sso expected proper motion along ra axis at the start time of the observation
arcsec/min
double
mu_de_1
sso expected proper motion along dec axis at the start time of the observation
arcsec/min
double
dist_dot_1
sso expected speed at the start time of the observation
km/s
double
pos1_deg_err
sso positional error at the start time of the observation
deg
double
ra_deg_2
sso positional error at the start time of the observation
double
dec_deg_2
sso expected declination (J2000) at the end time of the observation, end time computed as the start time plus duration of the observation
double
dist_2
expected distance to the sso from the satellite at the end time of the observation, end time computed as the start time plus duration of the observation
au
double
v_mag_2
sso expected magnitude V at the end time of the observation, end time computed as the start time plus duration of the observation
double
phase_2
sso expected phase angle at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
elong_2
sso expected elongation at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
mu_ra_cos_de_2
sso expected proper motion along ra axis at the end time of the observation, end time computed as the start time plus duration of the observation
arcsec/min
double
mu_de_2
sso expected proper motion along dec axis at the end time of the observation, end time computed as the start time plus duration of the observation
arcsec/min
double
dist_dot_2
expected sso distance to the sso from the satellite at the end time of the observation, end time computed as the start time plus duration of the observation
km/s
double
pos2_deg_err
sso expected positional error at the end time of the observation, end time computed as the start time plus duration of the observation
deg
double
xmatch_type
type of match (2: inside FoV;1: pos+error radius crossing FoV;3:sso path crossing FoV)
int
mlim_obs
limiting magnitude of the observation
double
v_mag_1_corrected
sso expected magnitude V at the start of the observation, zero-point corrected for the specific instrument filter
double
is_visible
flag indicating if corresponding detection is above limiting magnitude
boolean
tap_config
tap_config.coord_sys
epoch
char
equinox
char
id
char
system
char
xml_output
char
tap_config.properties
"key"
char
"value"
char
tap_descriptors
tap_descriptors.descriptors
category
char
intersect_polygon_query
boolean
mission
char
name
char
name_short
char
table_name
char
tap_descriptors.sso_extras
descriptor_table_name
char
xmatch_table
char
tap_schema
tap_schema.columns
arraysize
char
column_index
int
column_name
char
datatype
char
db_column_name
char
description
char
flags
int
indexed
int
principal
int
"public"
boolean
ref
char
schema_name
char
"size"
int
std
int
table_name
char
ucd
char
unit
char
utype
char
xtype
char
tap_schema.tables
table_name
table_name
TAP schema table name
tap_schema.functions
array_dims
char
array_type
char
description
char
function_name
char
"public"
boolean
return_type
char
schema_name
char
tap_schema.functions_arguments
all_functions_id
short
arg_order
int
arg_type
char
argument_name
char
arraysize
char
default_value
char
description
char
id
int
max_value
char
min_value
char
"public"
boolean
tap_schema.key_columns
from_column
char
key_id
char
target_column
char
tap_schema.keys
key_id
key_id
TAP schema key columns key id
tap_schema.keys
description
char
from_schema
char
from_table
char
key_id
char
"public"
boolean
target_schema
char
target_table
char
utype
char
tap_schema.tables
from_table
table_name
TAP schema keys from table
tap_schema.tables
target_table
table_name
TAP schema keys target table
tap_schema.schemas
db_schema_name
char
description
char
"public"
boolean
schema_index
int
schema_name
char
title
char
utype
char
tap_schema.tables
db_table_name
char
description
char
flags
int
hierarchy
char
"public"
boolean
schema_name
char
"size"
long
size_bytes
long
table_index
int
table_name
char
table_type
char
utype
char
tap_schema.schemas
schema_name
schema_name
TAP schema schema name
tap_upload