Further access options are discussed below
For a list of all services and tables belonging to this service's resource, see Information on resource 'AAVSO Photometric All Sky Survey (APASS) DR10'
You can access this service using:
This service is published as follows:
local means it is listed on our front page, ivo_managed means it has a record in the VO registry.
The following fields are available to provide input to the service (with some renderers, some of these fields may be unavailable):
| Name | Table Head | Description | Unit | UCD |
|---|---|---|---|---|
| DEC | Delta (ICRS) | Declination (ICRS decimal) | deg | pos.eq.dec |
| hscs_pos | Position/Name | Coordinates (as h m s, d m s or decimal degrees), or SIMBAD-resolvable object | N/A | N/A |
| hscs_sr | Search radius | Search radius in arcminutes | N/A | N/A |
| maxrec | Match limit | Maximum number of records returned. Pass 0 to retrieve service parameters. | N/A | N/A |
| RA | Alpha (ICRS) | Right Ascension (ICRS decimal) | deg | pos.eq.ra |
| responseformat | Output Format | File format requested for output. | N/A | meta.code.mime |
| SR | Search Radius | Search radius | deg | N/A |
| verb | Verbosity | Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. | N/A | N/A |
The following fields are contained in the output by default. More fields may be available for selection; these would be given below in the VOTable output fields.
| Name | Table Head | Description | Unit | UCD |
|---|---|---|---|---|
| _r | Dist. | Distance to cone center | deg | pos.angDistance |
| dec | Dec | ICRS declination for this object. | N/A | pos.eq.dec;meta.main |
| dec_error | Err. Dec | Estimated error in dec (there will be additional systematics especially in crowded fields). | deg | stat.error;pos.eq.dec |
| err_mag_b | Err B | Estimated error in mag_b. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.B |
| err_mag_g | Err g | Estimated error in mag_g. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.V |
| err_mag_i | Err i | Estimated error in mag_i. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.I |
| err_mag_r | Err r | Estimated error in mag_r. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.R |
| err_mag_u | Err u | Estimated error in mag_u. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.U |
| err_mag_v | Err V | Estimated error in mag_v. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.V |
| err_mag_y | Err Y | Estimated error in mag_y. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.I |
| err_mag_z_s | Err z_s | Estimated error in mag_z_s. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.I |
| id | Id | APASS DR10 identifier formed as (SPD zone)-(star number) | N/A | meta.id;meta.main |
| mag_b | Mag B | Magnitude in Johnson B (Vega system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.B |
| mag_g | Mag g | Magnitude in Sloan g' (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.V |
| mag_i | Mag i | Magnitude in Sloan i' (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.I |
| mag_r | Mag r | Magnitude in Sloan r' (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.R |
| mag_u | Mag u | Magnitude in Sloan u' (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.U |
| mag_v | Mag V | Magnitude in Johnson V (Vega system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.V |
| mag_y | Mag Y | Magnitude in Sloan Y (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.I |
| mag_z_s | Mag z_s | Magnitude in Sloan z_s (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.I |
| nobs_b | N(B) | Number of observations that went into mag_b | N/A | meta.number;obs;em.opt.B |
| nobs_g | N(g) | Number of observations that went into mag_g | N/A | meta.number;obs;em.opt.V |
| nobs_i | N(i) | Number of observations that went into mag_i | N/A | meta.number;obs;em.opt.I |
| nobs_r | N(r) | Number of observations that went into mag_r | N/A | meta.number;obs;em.opt.R |
| nobs_u | N(u) | Number of observations that went into mag_u | N/A | meta.number;obs;em.opt.U |
| nobs_v | N(V) | Number of observations that went into mag_v | N/A | meta.number;obs;em.opt.V |
| nobs_y | N(Y) | Number of observations that went into mag_y | N/A | meta.number;obs;em.opt.I |
| nobs_z_s | N(z_s) | Number of observations that went into mag_z_s | N/A | meta.number;obs;em.opt.I |
| ra | Ra | ICRS right ascension for this object. | N/A | pos.eq.ra;meta.main |
| ra_error | Err. RA | Estimated error in ra (there will be additional systematics especially in crowded fields). | deg | stat.error;pos.eq.ra |
The following fields are available in VOTable output. The verbosity level is a number intended to represent the relative importance of the field on a scale of 1 to 30. The services take a VERB argument. A field is included in the output if their verbosity level is less or equal VERB*10.
| Name | Table Head | Description | Unit | UCD | Verb. Level |
|---|---|---|---|---|---|
| id | Id | APASS DR10 identifier formed as (SPD zone)-(star number) | N/A | meta.id;meta.main | 1 |
| ra | Ra | ICRS right ascension for this object. | N/A | pos.eq.ra;meta.main | 1 |
| dec | Dec | ICRS declination for this object. | N/A | pos.eq.dec;meta.main | 1 |
| mag_b | Mag B | Magnitude in Johnson B (Vega system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.B | 5 |
| mag_v | Mag V | Magnitude in Johnson V (Vega system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.V | 5 |
| mag_u | Mag u | Magnitude in Sloan u' (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.U | 5 |
| mag_g | Mag g | Magnitude in Sloan g' (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.V | 5 |
| mag_r | Mag r | Magnitude in Sloan r' (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.R | 5 |
| mag_i | Mag i | Magnitude in Sloan i' (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.I | 5 |
| mag_z_s | Mag z_s | Magnitude in Sloan z_s (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.I | 5 |
| mag_y | Mag Y | Magnitude in Sloan Y (AB system). This is an aperture magnitude obtained with DAOPHOT. | mag | phot.mag;em.opt.I | 5 |
| _r | Dist. | Distance to cone center | deg | pos.angDistance | 10 |
| ra_error | Err. RA | Estimated error in ra (there will be additional systematics especially in crowded fields). | deg | stat.error;pos.eq.ra | 15 |
| dec_error | Err. Dec | Estimated error in dec (there will be additional systematics especially in crowded fields). | deg | stat.error;pos.eq.dec | 15 |
| nobs_b | N(B) | Number of observations that went into mag_b | N/A | meta.number;obs;em.opt.B | 15 |
| err_mag_b | Err B | Estimated error in mag_b. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.B | 15 |
| nobs_v | N(V) | Number of observations that went into mag_v | N/A | meta.number;obs;em.opt.V | 15 |
| err_mag_v | Err V | Estimated error in mag_v. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.V | 15 |
| nobs_u | N(u) | Number of observations that went into mag_u | N/A | meta.number;obs;em.opt.U | 15 |
| err_mag_u | Err u | Estimated error in mag_u. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.U | 15 |
| nobs_g | N(g) | Number of observations that went into mag_g | N/A | meta.number;obs;em.opt.V | 15 |
| err_mag_g | Err g | Estimated error in mag_g. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.V | 15 |
| nobs_r | N(r) | Number of observations that went into mag_r | N/A | meta.number;obs;em.opt.R | 15 |
| err_mag_r | Err r | Estimated error in mag_r. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.R | 15 |
| nobs_i | N(i) | Number of observations that went into mag_i | N/A | meta.number;obs;em.opt.I | 15 |
| err_mag_i | Err i | Estimated error in mag_i. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.I | 15 |
| nobs_z_s | N(z_s) | Number of observations that went into mag_z_s | N/A | meta.number;obs;em.opt.I | 15 |
| err_mag_z_s | Err z_s | Estimated error in mag_z_s. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.I | 15 |
| nobs_y | N(Y) | Number of observations that went into mag_y | N/A | meta.number;obs;em.opt.I | 15 |
| err_mag_y | Err Y | Estimated error in mag_y. From a comparison with DR9, it appears these estimates are overly pessimistic. | mag | stat.error;phot.mag;em.opt.I | 15 |
VOResource XML (that's something exclusively for VO nerds)