J/MNRAS/518/174/sourcesSources table is the main LSXPS tablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNObs? The number of observations covering the position of this source (NumObs)meta.numberintnullableNH1H? The hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH)cm**-2phys.columnDensitydoublenullablekTAH? The temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT)keVphys.temperaturedoublenullableE_FACU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullableLSXPSNumerical unique source identifier within LSXPS (LSXPS_ID)meta.id;meta.mainintIAUNameIAU-format name, LSXPS JHHMMSS s+-ddmmsss (IAUName)meta.idcharRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (Decl)degpos.eq.dec;meta.mainindexedErr90Position uncertainty, 90% confidence, radial, assumed to be Rayleigh-distributed (Err90)arcsecstat.errorfloatAProvenance of the astrometry used to derive the source position (AstromType) (1)meta.codeintGLONGalactic longitude (l)degpos.galactic.lonGLATGalactic latitude (b)degpos.galactic.latdoubleOffAxis? The mean angular distance of the source from the XRT boresight in all observations within which the source was detected (MeanOffAxisAngle)arcminpos.angDistance;stat.meanfloatnullableDNNThe distance to the closest LSXPS source to this one (NearestNeighbour)arcsecpos.angDistancedoubleDNNOKThe distance to the closest LSXPS source to this one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour)arcsecpos.angDistancedoubleNLSXPS? The LSXPS_ID of the closest LSXPS source to this one (NearestNeighbour_ID)meta.id.crossintnullableGoodNLSXPS? The LSXPS_ID of the closest LSXPS source to one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour_ID)meta.id.crossintnullableHPPIXThe Healpix pixel containing the source (NSIDE=128, ordering=RING) (HPPIX)meta.id;instrintt.exp? The total exposure at the source location in the catalogue (Exposure)stime.expointnullablet.start1The UTC date & time of the start of the first observation in LSXPS which covered the source location (FirstObsDate)stime.epochnullablet.stop1The UTC date & time of the end of the last observation in LSXPS which covered the source location (LastObsDate)stime.end;obsnullabletime.start1? The time of the start of the first observation in LSXPS which covered the source location, in Swift Mission Elapsed Time (FirstObsMET)stime.epochlongnullabletime.stop1? The time of the end of the last observation in LSXPS which covered the source location in, Swift Mission Elapsed Time (LastObsMET)stime.epochlongnullablet.start2The UTC date & time of the start of the first observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level (FirstDetDate)stime.epochnullablet.stop2The UTC date & time of the end of the last observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level (LastDetDate)stime.epochnullabletime.start2? The time of the start of the first observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (FirstDetMET)stime.epochlongnullabletime.stop2? The time of the end of the last observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (LastDetMET)stime.epochlongnullablet.start3The UTC date & time of the start of the first observation in LSXPS in which the source is detected in the blind search (FirstBlindDetDate)stime.epochnullablet.stop3The UTC date & time of the end of the last observation in LSXPS in which the source is detected in the blind search (LastBlindDetDate)stime.end;obsnullabletime.start3? The time of the start of the first observation in LSXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (FirstBlindDetMET)stime.epochlongnullabletime.stop3? The time of the end of the last observation in LSXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (LastBlindDetMET)stime.epochlongnullableNBlind? The number of observations in which this source was found in a blind search (NumBlindDetObs)meta.numberintnullableNDet? The number of observations in which this source is detected (NumDetObs)meta.numberintnullableIDBestThe ID of the 'best' detection, (cf the detection table) (BestDetectionID)meta.id.crossintF0? Whether the count-rate in the 0.3-10 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band0)meta.codeintnullableF1? Whether the count-rate in 0.3-1 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band1)meta.codeintnullableF2? Whether the count-rate in 1-2 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band2)meta.codeintnullableF3? Whether the count-rate in 2-10 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band3)meta.codeintnullableDetThe best detection flag from all detections of the source (DetFlag) (2)meta.codeintFFieldThe best field flag from all detections of the source (FieldFlag) (3)meta.codeintDet0The final detection flag 0.3-10 keV band (DetFlag_band0)meta.codeintDet1The final detection flag 0.3-1 keV band (DetFlag_band1)meta.codeintDet2The final detection flag in 1-2 keV band (DetFlag_band2)meta.codeintDet3The final detection flag in 2-10 keV band (DetFlag_band3)meta.codeintWarningThe worst optical loading warning from all detections of this source (OpticalLoadingWarning) (4)magphot.mag;em.optdoubleDetSLWWhether any detection of this source occurred within fitted stray light rings (StrayLightWarning)meta.codeintDetNBSWWhether any detection of this source occurred within the PSF wings of a bright object (NearBrightSourceWarning)meta.codeintDupWhether this source is potentially an alias (i e duplicate) of another source (IsPotentialAlias)meta.codeintAdDateThe date at which this source was added to LSXPS (WhenAdded)stime.epochnullableindexedSDetWhether the source was detected in the most recent observation of its location (StillDetected) (5)meta.codeintStatusA bit-wise flag describing the processing status of the source data (ProcessedStatus)meta.codeintModDateThe date at which this source was last analysed (WhenModified)stime.epochnullableCR0? The mean count-rate in 0.3-10 keV band (Rate_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableE_CR0? The 1-sigma positive uncertainty on the mean count-rate in the 0.3-10 keV band (Rate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_CR0[]? The 1-sigma negative uncertainty on the mean count-rate in 0.3-10 keV band (Rate_band0_neg)ct/sstat.errordoublenullableHR1? The aggregate HR1 hardness ratio of the source (HR1)phot.flux;arith.ratiofloatnullableE_HR1[]? The 1-sigma positive uncertainty on the aggregate HR1 hardness ratio of the source (HR1_pos)stat.error;stat.maxdoublenullablee_HR1[]? The 1-sigma negative uncertainty on the aggregate HR1 hardness ratio of the source (HR1_neg)stat.errordoublenullableHR2? The aggregate HR2 hardness ratio of the source (HR2)phot.flux;arith.ratiofloatnullableE_HR2[]? The 1-sigma positive uncertainty on the aggregate HR2 hardness ratio of the source (HR2_pos)stat.error;stat.maxdoublenullablee_HR2[]? The 1-sigma negative uncertainty on the aggregate HR2 hardness ratio of the source (HR2_neg)stat.errordoublenullableCR1? The mean count-rate in 0.3-1 keV band (Rate_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_CR1? The 1-sigma positive uncertainty on the mean count-rate in 0.3-1 keV band (Rate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_CR1[]? The 1-sigma negative uncertainty on the mean count-rate in 0.3-1 keV band (Rate_band1_neg)ct/sstat.errordoublenullableCR2? The mean count-rate in the 1-2 keV band (Rate_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_CR2? The 1-sigma positive uncertainty on the mean count-rate in the 1-2 keV band (Rate_band2_pos)ct/sstat.error;stat.maxdoublenullablee_CR2[]? The 1-sigma negative uncertainty on the mean count-rate in the 1-2 keV band (Rate_band2_neg)ct/sstat.errordoublenullableCR3? The mean count-rate in the 2-10 keV band (Rate_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullableE_CR3? The 1-sigma positive uncertainty on the mean count-rate in the 2-10 keV band (Rate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_CR3[]? The 1-sigma negative uncertainty on the mean count-rate in 2-10 keV band (Rate_band3_neg)ct/sstat.errordoublenullableCt0? The total number of counts in the source region in the 0.3-10 keV band (Counts_band0)ctphot.count;em.X-rayintnullableCt1? The total number of counts in the source region in the 0.3-1 keV band (Counts_band1)ctphot.count;em.X-ray.softintnullableCt2? The total number of counts in the source region in the 1-2 keV band (Counts_band2)ctphot.count;em.X-ray.softintnullableCt3? The total number of counts in the source region in the 2-10 keV band (Counts_band3)ctphot.count;em.X-ray.mediumintnullableBgCt0? The total number of background counts expected in the source region in 0.3-10 keV band (BgCounts_band0)ctphot.count;em.X-raydoublenullableBgCt1? The total number of background counts expected in the source region in the 0.3-1 keV band (BgCounts_band1)ctphot.count;em.X-ray.softdoublenullableBgCt2? The total number of background counts expected in the source region in the 1-2 keV band (BgCounts_band2)ctphot.count;em.X-ray.softdoublenullableBgCt3? The total number of background counts expected in the source region in the 2-10 keV band (BgCounts_band3)ctphot.count;em.X-ray.mediumdoublenullableCF0? The PSF correction factor in the 0.3-10 keV band (RateCF_band0)instr.paramdoublenullableCF1? The PSF correction factor in the 0.3-1 keV band (RateCF_band1)instr.paramdoublenullableCF2? The PSF correction factor in the 1-2 keV band (RateCF_band2)instr.paramdoublenullableCF3? The PSF correction factor in the 2-10 keV band (RateCF_band3)instr.paramdoublenullableFUL0? The 3-sigma upper confidence limit on the count-rate in the 0.3-10 keV band (UL_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableFUL1? The 3-sigma upper confidence limit on the count-rate in the 0.3-1 keV band (UL_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableFUL2? The 3-sigma upper confidence limit on the count-rate in the 1-2 keV band (UL_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableFUL3? The 3-sigma upper confidence limit on the count-rate in the 2-10 keV band (UL_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullablePCR0? The peak count-rate in 0.3-10 keV band (PeakRate_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableE_PCR0? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-10 keV band (PeakRate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_PCR0[]? The 1-sigma negative uncertainty on the peak count-rate in 0.3-10 keV band (PeakRate_band0_neg)ct/sstat.errordoublenullablePCR1? The peak count-rate in 0.3-1 keV band (PeakRate_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_PCR1? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-1 keV band (PeakRate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_PCR1[]? The 1-sigma negative uncertainty on the peak count-rate in 0.3-1 keV band (PeakRate_band1_neg)ct/sstat.errordoublenullablePCR2? The peak count-rate in the 1-2 keV band (PeakRate_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_PCR2? The 1-sigma positive uncertainty on the peak count-rate in the 1-2 keV band (PeakRate_band2_pos)ct/sstat.error;stat.maxdoublenullablee_PCR2[]? The 1-sigma negative uncertainty on the peak count-rate in the 1-2 keV band (PeakRate_band2_neg)ct/sstat.errordoublenullablePCR3? The peak count-rate in the 2-10 keV band (PeakRate_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullableE_PCR3? The 1-sigma positive uncertainty on the peak count-rate in the 2-10 keV band (PeakRate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_PCR3[]? The 1-sigma negative uncertainty on the peak count-rate in 2-10 keV band (PeakRate_band3_neg)ct/sstat.errordoublenullablePcstS0? The probability that the source count-rate in the 0.3-10 keV band does not vary between snapshots (PvarPchiSnapshot_band0)stat.fit.goodnessdoublenullablePcstS1? The probability that the source count-rate in the 0.3-1 keV band does not vary between snapshots (PvarPchiSnapshot_band1)stat.fit.goodnessdoublenullablePcstS2? The probability that the source count-rate in the 1-2 keV band does not vary between snapshots (PvarPchiSnapshot_band2)stat.fit.goodnessdoublenullablePcstS3? The probability that the source count-rate in the 2-10 keV band does not vary between snapshots (PvarPchiSnapshot_band3)stat.fit.goodnessdoublenullablePcstSHR1? The probability that the source HR1 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR1)stat.fit.goodnessdoublenullablePcstSHR2? The probability that the source HR2 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR2)stat.fit.goodnessdoublenullablePcst0? The probability that the source count-rate in the 0.3-10 keV band does not vary between observations (PvarPchiObsID_band0)stat.fit.goodnessdoublenullablePcst1? The probability that the source count-rate in the 0.3-1 keV band does not vary between observations (PvarPchiObsID_band1)stat.fit.goodnessdoublenullablePcst2? The probability that the source count-rate in the 1-2 keV band does not vary between observations (PvarPchiObsID_band2)stat.fit.goodnessdoublenullablePcst3? The probability that the source count-rate in the 2-10 keV band does not vary between observations (PvarPchiObsID_band3)stat.fit.goodnessdoublenullablePcstHR1? The probability that the source HR1 hardness ratio does not vary between observations (PvarPchiObsID_HR1)stat.fit.goodnessdoublenullablePcstHR2? The probability that the source HR2 hardness ratio does not vary between observations (PvarPchiObsID_HR2)stat.fit.goodnessdoublenullableNHgThe Galactic absorption column density (in cm-2) in the direction of the source, determined from Willingale et al (2013MNRAS.431..394W) (GalacticNH)cm**-2physdoublePow? Which of the available estimates of the power-law spectral ECF and fluxes (WhichPow) (6)meta.codeintnullableAPEC? Which of the available estimates of the APEC spectral ECF and fluxes (WhichAPEC) (7)meta.codeintnullableCFO0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming a power-law spectrum (PowECFO)mJ.m**-2.count**-1instr.paramdoublenullableCFU0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming a power-law spectrum (PowECFU)mJ.m**-2.count**-1instr.paramdoublenullableFPO0? The mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux_neg)mW.m**-2stat.errordoublenullableFPU0? The mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_neg)mW.m**-2stat.errordoublenullableECFO0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming an APEC spectrum (APECECFO)mJ.m**-2.count**-1instr.paramdoublenullableECFU0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming an APEC spectrum (APECECFU)mJ.m**-2.count**-1instr.paramdoublenullableFAO0? The mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux_neg)mW.m**-2stat.errordoublenullableFAU0? The mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_neg)mW.m**-2stat.errordoublenullableFpPO0? The peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpPO0? The 1-sigma positive uncertainty on the peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpPO0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux_neg)mW.m**-2stat.errordoublenullableFpPU0? The peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpPU0? The 1-sigma positive uncertainty on the peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpPU0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_neg)mW.m**-2stat.errordoublenullableFpAO0? The peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpAO0? The 1-sigma positive uncertainty on the peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpAO0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux_neg)mW.m**-2stat.errordoublenullableFpAU0? The peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpAU0? The 1-sigma positive uncertainty on the peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpAU0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_neg)mW.m**-2stat.errordoublenullableCECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the canned power-law spectrum (FixedPowECFO)mJ.m**-2.count**-1instr.paramdoublenullableCECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the canned power-law spectrum (FixedPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableFCOP0? The mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCOP0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCOP0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux_neg)mW.m**-2stat.errordoublenullableFCUP0? The mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCUP0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCUP0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableAECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the canned APEC spectrum (FixedAPECECFO)mJ.m**-2.count**-1instr.paramdoublenullableAECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the canned APEC spectrum (FixedAPECECFU)mJ.m**-2.count**-1instr.paramdoublenullableFCAO0? The mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCAO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCAO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_neg)mW.m**-2stat.errordoublenullableFCAU0? The mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCAU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCAU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullablePECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFO)mJ.m**-2.count**-1instr.paramdoublenullablePECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableE_NH1H[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH1H[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH_neg)cm**-2stat.errordoublenullableGam? The spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma)spect.indexdoublenullableE_Gam[]? The 1-sigma positive uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_pos)stat.error;stat.maxdoublenullablee_Gam[]? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_neg)stat.errordoublenullableFIPO0? The mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_neg)mW.m**-2stat.errordoublenullableFIPU0? The mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableIPECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFO)mJ.m**-2.count**-1instr.paramdoublenullableIPECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFU)mJ.m**-2.count**-1instr.paramdoublenullableNH2A? The hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH)cm**-2phys.columnDensitydoublenullableE_NH2A[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2A[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_neg)cm**-2stat.errordoublenullableE_kTAH[]? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT_pos)keVstat.error;stat.maxdoublenullablee_kTAH[]? The 1-sigma negative uncertainty on the temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT_neg)keVstat.errordoublenullableFAIO0? The mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAIO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAIO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_neg)mW.m**-2stat.errordoublenullableFAIU0? The mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAIU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAIU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullablePpow? The probability that the HR values of this source could be obtained if the true spectrum is an absorbed power-law (P_pow)stat.fit.goodnessfloatnullablePAPEC? The probability that the HR values of this source could be obtained if the true spectrum is an APEC (P_APEC)stat.fit.goodnessfloatnullableFPECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFO)mJ.m**-2.count**-1instr.paramdoublenullableFPECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableNH2C? The hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH)cm**-2phys.columnDensitydoublenullableE_NH2C[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2C[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_neg)cm**-2stat.errordoublenullableGamma? The spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma)spect.indexdoublenullableE_Gamma[]? The 1-sigma positive uncertainty on the spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma_pos)stat.error;stat.maxdoublenullablee_Gamma[]? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma_neg)stat.errordoublenullableFPCO0? The mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPCO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPCO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_neg)mW.m**-2stat.errordoublenullableFPCU0? The mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPCU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPCU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableCstat? The C-statistic from the power-law spectral fit to the custom-built spectrum (FittedPowCstat)stat.fit.paramfloatnullableDOF? The number of degrees of freedom in the power-law spectral fit to the custom-built spectrum (FittedPowDOF)meta.numberintnullableChi2r? The Churazov-weighted reduced chi^2 from the power-law spectral fit to the custom-built spectrum (FittedPowReducedChi2)stat.fit.chi2floatnullableACECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFO)mJ.m**-2.count**-1stat.fit.goodnessdoublenullableACECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFU)mJ.m**-2.count**-1stat.fit.goodnessdoublenullableNH2AC? The hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH)cm**-2phys.columnDensitydoublenullableE_NH2AC[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2AC[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_neg)cm**-2stat.errordoublenullablekTAC? The temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT)keVphys.temperaturedoublenullableE_kTAC[]? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_pos)keVstat.error;stat.maxdoublenullablee_kTAC[]? The 1-sigma negative uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_neg)keVstat.errordoublenullableFACO0? The mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FACO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FACO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_neg)mW.m**-2stat.errordoublenullableFACU0? The mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullablee_FACU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullableCstatA? The C-statistic from the APEC spectral fit to the custom-built spectrum (FittedAPECCstat)stat.fit.paramdoublenullableDOFA? The number of degrees of freedom in the APEC spectral fit to the custom-built spectrum (FittedAPECDOF)meta.numberintnullableChi2rA? The Churazov-weighted reduced chi^2 from the APEC spectral fit to the custom-built spectrum (FittedAPECReducedChi2)stat.fit.chi2floatnullableHasSpecWhether a custom-built spectrum was created for this source (HasSpec)meta.codeintNExt? The number of external sources found to agree spatially with this one at the 3-sigma level (NumExternalMatches)meta.codeintnullableNExt2? The number of external sources found to agree spatially with this one at the 3-sigma level, excluding 2MASS and USNO-B1 matches (NumExternalMatches_slim)meta.codeintnullableROSHRIWhether the source is spatially within 3 sigma of a source in the Rosat HRI catalogue (Cat. IX/28) (MatchInROSHRI)meta.codeint2RXSWhether the source is spatially within 3 sigma of a source in the 2RXS catalogue (Cat. J/A+A/588/A103) (MatchIn2RXS)meta.codeint3XMMDR8Whether the source is spatially within 3 sigma of a source in the 3XMM-DR8 catalogue (Cat. IX/55) (MatchIn4XMM_DR10)meta.codeint3XMMDR7sWhether the source is spatially within 3 sigma of a source in the 3XMM-DR7s (stacked) catalogue (Cat. IX/56) (MatchIn4XMM_DR10s)meta.codeintXMMSL2Whether the source is spatially within 3 sigma of a source in the XMMSL2 catalogue (Cat. IX/53) (MatchInXMMSL2)meta.codeintSwiftFTWhether the source is spatially within 3 sigma of a source in the SwiftFT catalog (Cat. J/A+A/528/A122) (MatchInSwiftFT)meta.codeint1SWXRTWhether the source is spatially within 3 sigma of a source in the 1SWXRT catalogue (Cat. J/A+A/551/A142) (MatchIn1SWXRT)meta.codeintXRTGRBWhether the source is spatially within 3 sigma of an XRT GRB afterglow (MatchInXRTGRB)meta.codeintSDSSQSOWhether the source is spatially within 3 sigma of a source in the SDSS QSO DR14 catalogue (MatchInSDSS_QSO_DR14)meta.codeint2MASSWhether the source is spatially within 3 sigma of a source in the 2MASS catalogue (Cat. II/246) (MatchIn2MASS)meta.codeintUSNOB1Whether the source is spatially within 3 sigma of a source in the USNO-B1 catalogue (Cat. I/284) (MatchInUSNOB1)meta.codeint2CSCWhether the source is spatially within 3 sigma of a source in the 2CSC catalogue (MatchIn2CSC)meta.codeint2SXPSWhether the source is spatially within 3 sigma of a source in the 2SXPS (Cat. IX/58) catalogue (MatchIn2SXPS)meta.codeint
J/MNRAS/518/174/scleanClean subset of the source table those with a best Det Flag of 0 or 1 for Good or ReasonableErr90Position uncertainty, 90% confidence, radial, assumed to be Rayleigh-distributed (Err90)arcsecstat.errorfloatGLONGalactic longitude (l)degpos.galactic.lonDetNBSWWhether any detection of this source occurred within the PSF wings of a bright object (NearBrightSourceWarning)meta.codeintE_CR2? The 1-sigma positive uncertainty on the mean count-rate in the 1-2 keV band (Rate_band2_pos)ct/sstat.error;stat.maxdoublenullableFUL2? The 3-sigma upper confidence limit on the count-rate in the 1-2 keV band (UL_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullablePow? Which of the available estimates of the power-law spectral ECF and fluxes (WhichPow) (6)meta.codeintnullablee_FpPU0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_neg)mW.m**-2stat.errordoublenullableCstat? The C-statistic from the power-law spectral fit to the custom-built spectrum (FittedPowCstat)stat.fit.paramfloatnullableChi2rA? The Churazov-weighted reduced chi^2 from the APEC spectral fit to the custom-built spectrum (FittedAPECReducedChi2)stat.fit.chi2floatnullableHasSpecWhether a custom-built spectrum was created for this source (HasSpec)meta.codeintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLSXPSNumerical unique source identifier within LSXPS (LSXPS_ID)meta.id;meta.mainintRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (Decl)degpos.eq.dec;meta.mainindexedAProvenance of the astrometry used to derive the source position (AstromType) (1)meta.codeintGLATGalactic latitude (b)degpos.galactic.latdoubleOffAxis? The mean angular distance of the source from the XRT boresight in all observations within which the source was detected (MeanOffAxisAngle)arcminpos.angDistance;stat.meanfloatnullableDNNThe distance to the closest LSXPS source to this one (NearestNeighbour)arcsecpos.angDistancedoubleDNNOKThe distance to the closest LSXPS source to this one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour)arcsecpos.angDistancedoubleNLSXPS? The LSXPS_ID of the closest LSXPS source to this one (NearestNeighbour_ID)meta.id.crossintnullableGoodNLSXPS? The LSXPS_ID of the closest LSXPS source to one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour_ID)meta.id.crossintnullableHPPIXThe Healpix pixel containing the source (NSIDE=128, ordering=RING) (HPPIX)meta.id;instrintt.exp? The total exposure at the source location in the catalogue (Exposure)stime.expointnullablet.start1The UTC date & time of the start of the first observation in LSXPS which covered the source location (FirstObsDate)stime.epochnullablet.stop1The UTC date & time of the end of the last observation in LSXPS which covered the source location (LastObsDate)stime.end;obsnullabletime.start1? The time of the start of the first observation in LSXPS which covered the source location, in Swift Mission Elapsed Time (FirstObsMET)stime.epochlongnullabletime.stop1? The time of the end of the last observation in LSXPS which covered the source location in, Swift Mission Elapsed Time (LastObsMET)stime.epochlongnullablet.start2The UTC date & time of the start of the first observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level (FirstDetDate)stime.epochnullablet.stop2The UTC date & time of the end of the last observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level (LastDetDate)stime.epochnullabletime.start2? The time of the start of the first observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (FirstDetMET)stime.epochlongnullabletime.stop2? The time of the end of the last observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (LastDetMET)stime.epochlongnullablet.start3The UTC date & time of the start of the first observation in LSXPS in which the source is detected in the blind search (FirstBlindDetDate)stime.epochnullablet.stop3The UTC date & time of the end of the last observation in LSXPS in which the source is detected in the blind search (LastBlindDetDate)stime.end;obsnullabletime.start3? The time of the start of the first observation in LSXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (FirstBlindDetMET)stime.epochlongnullabletime.stop3? The time of the end of the last observation in LSXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (LastBlindDetMET)stime.epochlongnullableNObs? The number of observations covering the position of this source (NumObs)meta.numberintnullableNBlind? The number of observations in which this source was found in a blind search (NumBlindDetObs)meta.numberintnullableNDet? The number of observations in which this source is detected (NumDetObs)meta.numberintnullableIDBestThe ID of the 'best' detection, (cf the detection table) (BestDetectionID)meta.id.crossintF0? Whether the count-rate in the 0.3-10 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band0)meta.codeintnullableF1? Whether the count-rate in 0.3-1 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band1)meta.codeintnullableF2? Whether the count-rate in 1-2 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band2)meta.codeintnullableF3? Whether the count-rate in 2-10 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band3)meta.codeintnullableDetThe best detection flag from all detections of the source (DetFlag) (2)meta.codeintFFieldThe best field flag from all detections of the source (FieldFlag) (3)meta.codeintDet0The final detection flag 0.3-10 keV band (DetFlag_band0)meta.codeintDet1The final detection flag 0.3-1 keV band (DetFlag_band1)meta.codeintDet2The final detection flag in 1-2 keV band (DetFlag_band2)meta.codeintDet3The final detection flag in 2-10 keV band (DetFlag_band3)meta.codeintWarningThe worst optical loading warning from all detections of this source (OpticalLoadingWarning) (4)magphot.mag;em.optdoubleDetSLWWhether any detection of this source occurred within fitted stray light rings (StrayLightWarning)meta.codeintDupWhether this source is potentially an alias (i e duplicate) of another source (IsPotentialAlias)meta.codeintAdDateThe date at which this source was added to LSXPS (WhenAdded)stime.epochnullableindexedSDetWhether the source was detected in the most recent observation of its location (StillDetected) (5)meta.codeintStatusA bit-wise flag describing the processing status of the source data (ProcessedStatus)meta.codeintModDateThe date at which this source was last analysed (WhenModified)stime.epochnullableCR0? The mean count-rate in 0.3-10 keV band (Rate_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableE_CR0? The 1-sigma positive uncertainty on the mean count-rate in the 0.3-10 keV band (Rate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_CR0[]? The 1-sigma negative uncertainty on the mean count-rate in 0.3-10 keV band (Rate_band0_neg)ct/sstat.errordoublenullableHR1? The aggregate HR1 hardness ratio of the source (HR1)phot.flux;arith.ratiofloatnullableE_HR1[]? The 1-sigma positive uncertainty on the aggregate HR1 hardness ratio of the source (HR1_pos)stat.error;stat.maxdoublenullablee_HR1[]? The 1-sigma negative uncertainty on the aggregate HR1 hardness ratio of the source (HR1_neg)stat.errordoublenullableHR2? The aggregate HR2 hardness ratio of the source (HR2)phot.flux;arith.ratiofloatnullableE_HR2[]? The 1-sigma positive uncertainty on the aggregate HR2 hardness ratio of the source (HR2_pos)stat.error;stat.maxdoublenullablee_HR2[]? The 1-sigma negative uncertainty on the aggregate HR2 hardness ratio of the source (HR2_neg)stat.errordoublenullableCR1? The mean count-rate in 0.3-1 keV band (Rate_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_CR1? The 1-sigma positive uncertainty on the mean count-rate in 0.3-1 keV band (Rate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_CR1[]? The 1-sigma negative uncertainty on the mean count-rate in 0.3-1 keV band (Rate_band1_neg)ct/sstat.errordoublenullableCR2? The mean count-rate in the 1-2 keV band (Rate_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullablee_CR2[]? The 1-sigma negative uncertainty on the mean count-rate in the 1-2 keV band (Rate_band2_neg)ct/sstat.errordoublenullableCR3? The mean count-rate in the 2-10 keV band (Rate_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullableE_CR3? The 1-sigma positive uncertainty on the mean count-rate in the 2-10 keV band (Rate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_CR3[]? The 1-sigma negative uncertainty on the mean count-rate in 2-10 keV band (Rate_band3_neg)ct/sstat.errordoublenullableCt0? The total number of counts in the source region in the 0.3-10 keV band (Counts_band0)ctphot.count;em.X-rayintnullableCt1? The total number of counts in the source region in the 0.3-1 keV band (Counts_band1)ctphot.count;em.X-ray.softintnullableCt2? The total number of counts in the source region in the 1-2 keV band (Counts_band2)ctphot.count;em.X-ray.softintnullableCt3? The total number of counts in the source region in the 2-10 keV band (Counts_band3)ctphot.count;em.X-ray.mediumintnullableBgCt0? The total number of background counts expected in the source region in 0.3-10 keV band (BgCounts_band0)ctphot.count;em.X-raydoublenullableBgCt1? The total number of background counts expected in the source region in the 0.3-1 keV band (BgCounts_band1)ctphot.count;em.X-ray.softdoublenullableBgCt2? The total number of background counts expected in the source region in the 1-2 keV band (BgCounts_band2)ctphot.count;em.X-ray.softdoublenullableBgCt3? The total number of background counts expected in the source region in the 2-10 keV band (BgCounts_band3)ctphot.count;em.X-ray.mediumdoublenullableCF0? The PSF correction factor in the 0.3-10 keV band (RateCF_band0)instr.paramdoublenullableCF1? The PSF correction factor in the 0.3-1 keV band (RateCF_band1)instr.paramdoublenullableCF2? The PSF correction factor in the 1-2 keV band (RateCF_band2)instr.paramdoublenullableCF3? The PSF correction factor in the 2-10 keV band (RateCF_band3)instr.paramdoublenullableFUL0? The 3-sigma upper confidence limit on the count-rate in the 0.3-10 keV band (UL_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableFUL1? The 3-sigma upper confidence limit on the count-rate in the 0.3-1 keV band (UL_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableFUL3? The 3-sigma upper confidence limit on the count-rate in the 2-10 keV band (UL_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullablePCR0? The peak count-rate in 0.3-10 keV band (PeakRate_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableE_PCR0? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-10 keV band (PeakRate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_PCR0[]? The 1-sigma negative uncertainty on the peak count-rate in 0.3-10 keV band (PeakRate_band0_neg)ct/sstat.errordoublenullablePCR1? The peak count-rate in 0.3-1 keV band (PeakRate_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_PCR1? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-1 keV band (PeakRate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_PCR1[]? The 1-sigma negative uncertainty on the peak count-rate in 0.3-1 keV band (PeakRate_band1_neg)ct/sstat.errordoublenullablePCR2? The peak count-rate in the 1-2 keV band (PeakRate_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_PCR2? The 1-sigma positive uncertainty on the peak count-rate in the 1-2 keV band (PeakRate_band2_pos)ct/sstat.error;stat.maxdoublenullablee_PCR2[]? The 1-sigma negative uncertainty on the peak count-rate in the 1-2 keV band (PeakRate_band2_neg)ct/sstat.errordoublenullablePCR3? The peak count-rate in the 2-10 keV band (PeakRate_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullableE_PCR3? The 1-sigma positive uncertainty on the peak count-rate in the 2-10 keV band (PeakRate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_PCR3[]? The 1-sigma negative uncertainty on the peak count-rate in 2-10 keV band (PeakRate_band3_neg)ct/sstat.errordoublenullablePcstS0? The probability that the source count-rate in the 0.3-10 keV band does not vary between snapshots (PvarPchiSnapshot_band0)stat.fit.goodnessdoublenullablePcstS1? The probability that the source count-rate in the 0.3-1 keV band does not vary between snapshots (PvarPchiSnapshot_band1)stat.fit.goodnessdoublenullablePcstS2? The probability that the source count-rate in the 1-2 keV band does not vary between snapshots (PvarPchiSnapshot_band2)stat.fit.goodnessdoublenullablePcstS3? The probability that the source count-rate in the 2-10 keV band does not vary between snapshots (PvarPchiSnapshot_band3)stat.fit.goodnessdoublenullablePcstSHR1? The probability that the source HR1 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR1)stat.fit.goodnessdoublenullablePcstSHR2? The probability that the source HR2 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR2)stat.fit.goodnessdoublenullablePcst0? The probability that the source count-rate in the 0.3-10 keV band does not vary between observations (PvarPchiObsID_band0)stat.fit.goodnessdoublenullablePcst1? The probability that the source count-rate in the 0.3-1 keV band does not vary between observations (PvarPchiObsID_band1)stat.fit.goodnessdoublenullablePcst2? The probability that the source count-rate in the 1-2 keV band does not vary between observations (PvarPchiObsID_band2)stat.fit.goodnessdoublenullablePcst3? The probability that the source count-rate in the 2-10 keV band does not vary between observations (PvarPchiObsID_band3)stat.fit.goodnessdoublenullablePcstHR1? The probability that the source HR1 hardness ratio does not vary between observations (PvarPchiObsID_HR1)stat.fit.goodnessdoublenullablePcstHR2? The probability that the source HR2 hardness ratio does not vary between observations (PvarPchiObsID_HR2)stat.fit.goodnessdoublenullableNHgThe Galactic absorption column density (in cm-2) in the direction of the source, determined from Willingale et al (2013MNRAS.431..394W) (GalacticNH)cm**-2physdoubleAPEC? Which of the available estimates of the APEC spectral ECF and fluxes (WhichAPEC) (7)meta.codeintnullableCFO0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming a power-law spectrum (PowECFO)mJ.m**-2.count**-1instr.paramdoublenullableCFU0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming a power-law spectrum (PowECFU)mJ.m**-2.count**-1instr.paramdoublenullableFPO0? The mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux_neg)mW.m**-2stat.errordoublenullableFPU0? The mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_neg)mW.m**-2stat.errordoublenullableECFO0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming an APEC spectrum (APECECFO)mJ.m**-2.count**-1instr.paramdoublenullableECFU0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming an APEC spectrum (APECECFU)mJ.m**-2.count**-1instr.paramdoublenullableFAO0? The mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux_neg)mW.m**-2stat.errordoublenullableFAU0? The mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_neg)mW.m**-2stat.errordoublenullableFpPO0? The peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpPO0? The 1-sigma positive uncertainty on the peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpPO0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux_neg)mW.m**-2stat.errordoublenullableFpPU0? The peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpPU0? The 1-sigma positive uncertainty on the peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullableFpAO0? The peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpAO0? The 1-sigma positive uncertainty on the peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpAO0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux_neg)mW.m**-2stat.errordoublenullableFpAU0? The peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpAU0? The 1-sigma positive uncertainty on the peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpAU0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_neg)mW.m**-2stat.errordoublenullableCECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the canned power-law spectrum (FixedPowECFO)mJ.m**-2.count**-1instr.paramdoublenullableCECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the canned power-law spectrum (FixedPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableFCOP0? The mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCOP0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCOP0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux_neg)mW.m**-2stat.errordoublenullableFCUP0? The mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCUP0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCUP0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableAECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the canned APEC spectrum (FixedAPECECFO)mJ.m**-2.count**-1instr.paramdoublenullableAECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the canned APEC spectrum (FixedAPECECFU)mJ.m**-2.count**-1instr.paramdoublenullableFCAO0? The mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCAO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCAO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_neg)mW.m**-2stat.errordoublenullableFCAU0? The mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCAU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCAU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullablePECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFO)mJ.m**-2.count**-1instr.paramdoublenullablePECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableNH1H? The hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH)cm**-2phys.columnDensitydoublenullableE_NH1H[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH1H[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH_neg)cm**-2stat.errordoublenullableGam? The spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma)spect.indexdoublenullableE_Gam[]? The 1-sigma positive uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_pos)stat.error;stat.maxdoublenullablee_Gam[]? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_neg)stat.errordoublenullableFIPO0? The mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_neg)mW.m**-2stat.errordoublenullableFIPU0? The mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableIPECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFO)mJ.m**-2.count**-1instr.paramdoublenullableIPECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFU)mJ.m**-2.count**-1instr.paramdoublenullableNH2A? The hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH)cm**-2phys.columnDensitydoublenullableE_NH2A[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2A[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_neg)cm**-2stat.errordoublenullablekTAH? The temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT)keVphys.temperaturedoublenullableE_kTAH[]? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT_pos)keVstat.error;stat.maxdoublenullablee_kTAH[]? The 1-sigma negative uncertainty on the temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT_neg)keVstat.errordoublenullableFAIO0? The mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAIO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAIO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_neg)mW.m**-2stat.errordoublenullableFAIU0? The mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAIU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAIU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullablePpow? The probability that the HR values of this source could be obtained if the true spectrum is an absorbed power-law (P_pow)stat.fit.goodnessfloatnullablePAPEC? The probability that the HR values of this source could be obtained if the true spectrum is an APEC (P_APEC)stat.fit.goodnessfloatnullableFPECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFO)mJ.m**-2.count**-1instr.paramdoublenullableFPECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableNH2C? The hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH)cm**-2phys.columnDensitydoublenullableE_NH2C[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2C[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_neg)cm**-2stat.errordoublenullableGamma? The spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma)spect.indexdoublenullableE_Gamma[]? The 1-sigma positive uncertainty on the spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma_pos)stat.error;stat.maxdoublenullablee_Gamma[]? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma_neg)stat.errordoublenullableFPCO0? The mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPCO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPCO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_neg)mW.m**-2stat.errordoublenullableFPCU0? The mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPCU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPCU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableDOF? The number of degrees of freedom in the power-law spectral fit to the custom-built spectrum (FittedPowDOF)meta.numberintnullableChi2r? The Churazov-weighted reduced chi^2 from the power-law spectral fit to the custom-built spectrum (FittedPowReducedChi2)stat.fit.chi2floatnullableACECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFO)mJ.m**-2.count**-1stat.fit.goodnessdoublenullableACECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFU)mJ.m**-2.count**-1stat.fit.goodnessdoublenullableNH2AC? The hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH)cm**-2phys.columnDensitydoublenullableE_NH2AC[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2AC[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_neg)cm**-2stat.errordoublenullablekTAC? The temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT)keVphys.temperaturedoublenullableE_kTAC[]? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_pos)keVstat.error;stat.maxdoublenullablee_kTAC[]? The 1-sigma negative uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_neg)keVstat.errordoublenullableFACO0? The mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FACO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FACO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_neg)mW.m**-2stat.errordoublenullableFACU0? The mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FACU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FACU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullableCstatA? The C-statistic from the APEC spectral fit to the custom-built spectrum (FittedAPECCstat)stat.fit.paramdoublenullableDOFA? The number of degrees of freedom in the APEC spectral fit to the custom-built spectrum (FittedAPECDOF)meta.numberintnullableNExt? The number of external sources found to agree spatially with this one at the 3-sigma level (NumExternalMatches)meta.codeintnullableNExt2? The number of external sources found to agree spatially with this one at the 3-sigma level, excluding 2MASS and USNO-B1 matches (NumExternalMatches_slim)meta.codeintnullableROSHRIWhether the source is spatially within 3 sigma of a source in the Rosat HRI catalogue (Cat. IX/28) (MatchInROSHRI)meta.codeint2RXSWhether the source is spatially within 3 sigma of a source in the 2RXS catalogue (Cat. J/A+A/588/A103) (MatchIn2RXS)meta.codeint3XMMDR8Whether the source is spatially within 3 sigma of a source in the 3XMM-DR8 catalogue (Cat. IX/55) (MatchIn4XMM_DR10)meta.codeint3XMMDR7sWhether the source is spatially within 3 sigma of a source in the 3XMM-DR7s (stacked) catalogue (Cat. IX/56) (MatchIn4XMM_DR10s)meta.codeintXMMSL2Whether the source is spatially within 3 sigma of a source in the XMMSL2 catalogue (Cat. IX/53) (MatchInXMMSL2)meta.codeintSwiftFTWhether the source is spatially within 3 sigma of a source in the SwiftFT catalog (Cat. J/A+A/528/A122) (MatchInSwiftFT)meta.codeint1SWXRTWhether the source is spatially within 3 sigma of a source in the 1SWXRT catalogue (Cat. J/A+A/551/A142) (MatchIn1SWXRT)meta.codeintXRTGRBWhether the source is spatially within 3 sigma of an XRT GRB afterglow (MatchInXRTGRB)meta.codeintSDSSQSOWhether the source is spatially within 3 sigma of a source in the SDSS QSO DR14 catalogue (MatchInSDSS_QSO_DR14)meta.codeint2MASSWhether the source is spatially within 3 sigma of a source in the 2MASS catalogue (Cat. II/246) (MatchIn2MASS)meta.codeintUSNOB1Whether the source is spatially within 3 sigma of a source in the USNO-B1 catalogue (Cat. I/284) (MatchInUSNOB1)meta.codeint2CSCWhether the source is spatially within 3 sigma of a source in the 2CSC catalogue (MatchIn2CSC)meta.codeint2SXPSWhether the source is spatially within 3 sigma of a source in the 2SXPS (Cat. IX/58) catalogue (MatchIn2SXPS)meta.codeintIAUNameIAU-format name, LSXPS JHHMMSS s+-ddmmsss (IAUName)meta.idchar
J/MNRAS/518/174/sucleanUltraclean subset of the sclean table those with Det=0 and FField=0F0? Whether the count-rate in the 0.3-10 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band0)meta.codeintnullableDetThe best detection flag from all detections of the source (DetFlag) (2)meta.codeintE_FPU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullableE_Gam[]? The 1-sigma positive uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_pos)stat.error;stat.maxdoublenullableE_FAIU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLSXPSNumerical unique source identifier within LSXPS (LSXPS_ID)meta.id;meta.mainintIAUNameIAU-format name, LSXPS JHHMMSS s+-ddmmsss (IAUName)meta.idcharRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (Decl)degpos.eq.dec;meta.mainindexedErr90Position uncertainty, 90% confidence, radial, assumed to be Rayleigh-distributed (Err90)arcsecstat.errorfloatAProvenance of the astrometry used to derive the source position (AstromType) (1)meta.codeintGLONGalactic longitude (l)degpos.galactic.lonGLATGalactic latitude (b)degpos.galactic.latdoubleOffAxis? The mean angular distance of the source from the XRT boresight in all observations within which the source was detected (MeanOffAxisAngle)arcminpos.angDistance;stat.meanfloatnullableDNNThe distance to the closest LSXPS source to this one (NearestNeighbour)arcsecpos.angDistancedoubleDNNOKThe distance to the closest LSXPS source to this one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour)arcsecpos.angDistancedoubleNLSXPS? The LSXPS_ID of the closest LSXPS source to this one (NearestNeighbour_ID)meta.id.crossintnullableGoodNLSXPS? The LSXPS_ID of the closest LSXPS source to one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour_ID)meta.id.crossintnullableHPPIXThe Healpix pixel containing the source (NSIDE=128, ordering=RING) (HPPIX)meta.id;instrintt.exp? The total exposure at the source location in the catalogue (Exposure)stime.expointnullablet.start1The UTC date & time of the start of the first observation in LSXPS which covered the source location (FirstObsDate)stime.epochnullablet.stop1The UTC date & time of the end of the last observation in LSXPS which covered the source location (LastObsDate)stime.end;obsnullabletime.start1? The time of the start of the first observation in LSXPS which covered the source location, in Swift Mission Elapsed Time (FirstObsMET)stime.epochlongnullabletime.stop1? The time of the end of the last observation in LSXPS which covered the source location in, Swift Mission Elapsed Time (LastObsMET)stime.epochlongnullablet.start2The UTC date & time of the start of the first observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level (FirstDetDate)stime.epochnullablet.stop2The UTC date & time of the end of the last observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level (LastDetDate)stime.epochnullabletime.start2? The time of the start of the first observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (FirstDetMET)stime.epochlongnullabletime.stop2? The time of the end of the last observation in LSXPS in which the source count rate is inconsisent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (LastDetMET)stime.epochlongnullablet.start3The UTC date & time of the start of the first observation in LSXPS in which the source is detected in the blind search (FirstBlindDetDate)stime.epochnullablet.stop3The UTC date & time of the end of the last observation in LSXPS in which the source is detected in the blind search (LastBlindDetDate)stime.end;obsnullabletime.start3? The time of the start of the first observation in LSXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (FirstBlindDetMET)stime.epochlongnullabletime.stop3? The time of the end of the last observation in LSXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (LastBlindDetMET)stime.epochlongnullableNObs? The number of observations covering the position of this source (NumObs)meta.numberintnullableNBlind? The number of observations in which this source was found in a blind search (NumBlindDetObs)meta.numberintnullableNDet? The number of observations in which this source is detected (NumDetObs)meta.numberintnullableIDBestThe ID of the 'best' detection, (cf the detection table) (BestDetectionID)meta.id.crossintF1? Whether the count-rate in 0.3-1 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band1)meta.codeintnullableF2? Whether the count-rate in 1-2 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band2)meta.codeintnullableF3? Whether the count-rate in 2-10 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band3)meta.codeintnullableFFieldThe best field flag from all detections of the source (FieldFlag) (3)meta.codeintDet0The final detection flag 0.3-10 keV band (DetFlag_band0)meta.codeintDet1The final detection flag 0.3-1 keV band (DetFlag_band1)meta.codeintDet2The final detection flag in 1-2 keV band (DetFlag_band2)meta.codeintDet3The final detection flag in 2-10 keV band (DetFlag_band3)meta.codeintWarningThe worst optical loading warning from all detections of this source (OpticalLoadingWarning) (4)magphot.mag;em.optdoubleDetSLWWhether any detection of this source occurred within fitted stray light rings (StrayLightWarning)meta.codeintDetNBSWWhether any detection of this source occurred within the PSF wings of a bright object (NearBrightSourceWarning)meta.codeintDupWhether this source is potentially an alias (i e duplicate) of another source (IsPotentialAlias)meta.codeintSDetWhether the source was detected in the most recent observation of its location (StillDetected) (5)meta.codeintStatusA bit-wise flag describing the processing status of the source data (ProcessedStatus)meta.codeintModDateThe date at which this source was last analysed (WhenModified)stime.epochnullableCR0? The mean count-rate in 0.3-10 keV band (Rate_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableE_CR0? The 1-sigma positive uncertainty on the mean count-rate in the 0.3-10 keV band (Rate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_CR0[]? The 1-sigma negative uncertainty on the mean count-rate in 0.3-10 keV band (Rate_band0_neg)ct/sstat.errordoublenullableHR1? The aggregate HR1 hardness ratio of the source (HR1)phot.flux;arith.ratiofloatnullableE_HR1[]? The 1-sigma positive uncertainty on the aggregate HR1 hardness ratio of the source (HR1_pos)stat.error;stat.maxdoublenullablee_HR1[]? The 1-sigma negative uncertainty on the aggregate HR1 hardness ratio of the source (HR1_neg)stat.errordoublenullableHR2? The aggregate HR2 hardness ratio of the source (HR2)phot.flux;arith.ratiofloatnullableE_HR2[]? The 1-sigma positive uncertainty on the aggregate HR2 hardness ratio of the source (HR2_pos)stat.error;stat.maxdoublenullablee_HR2[]? The 1-sigma negative uncertainty on the aggregate HR2 hardness ratio of the source (HR2_neg)stat.errordoublenullableCR1? The mean count-rate in 0.3-1 keV band (Rate_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_CR1? The 1-sigma positive uncertainty on the mean count-rate in 0.3-1 keV band (Rate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_CR1[]? The 1-sigma negative uncertainty on the mean count-rate in 0.3-1 keV band (Rate_band1_neg)ct/sstat.errordoublenullableCR2? The mean count-rate in the 1-2 keV band (Rate_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_CR2? The 1-sigma positive uncertainty on the mean count-rate in the 1-2 keV band (Rate_band2_pos)ct/sstat.error;stat.maxdoublenullablee_CR2[]? The 1-sigma negative uncertainty on the mean count-rate in the 1-2 keV band (Rate_band2_neg)ct/sstat.errordoublenullableCR3? The mean count-rate in the 2-10 keV band (Rate_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullableE_CR3? The 1-sigma positive uncertainty on the mean count-rate in the 2-10 keV band (Rate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_CR3[]? The 1-sigma negative uncertainty on the mean count-rate in 2-10 keV band (Rate_band3_neg)ct/sstat.errordoublenullableCt0? The total number of counts in the source region in the 0.3-10 keV band (Counts_band0)ctphot.count;em.X-rayintnullableCt1? The total number of counts in the source region in the 0.3-1 keV band (Counts_band1)ctphot.count;em.X-ray.softintnullableCt2? The total number of counts in the source region in the 1-2 keV band (Counts_band2)ctphot.count;em.X-ray.softintnullableCt3? The total number of counts in the source region in the 2-10 keV band (Counts_band3)ctphot.count;em.X-ray.mediumintnullableBgCt0? The total number of background counts expected in the source region in 0.3-10 keV band (BgCounts_band0)ctphot.count;em.X-raydoublenullableBgCt1? The total number of background counts expected in the source region in the 0.3-1 keV band (BgCounts_band1)ctphot.count;em.X-ray.softdoublenullableBgCt2? The total number of background counts expected in the source region in the 1-2 keV band (BgCounts_band2)ctphot.count;em.X-ray.softdoublenullableBgCt3? The total number of background counts expected in the source region in the 2-10 keV band (BgCounts_band3)ctphot.count;em.X-ray.mediumdoublenullableCF0? The PSF correction factor in the 0.3-10 keV band (RateCF_band0)instr.paramdoublenullableCF1? The PSF correction factor in the 0.3-1 keV band (RateCF_band1)instr.paramdoublenullableCF2? The PSF correction factor in the 1-2 keV band (RateCF_band2)instr.paramdoublenullableCF3? The PSF correction factor in the 2-10 keV band (RateCF_band3)instr.paramdoublenullableFUL0? The 3-sigma upper confidence limit on the count-rate in the 0.3-10 keV band (UL_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableFUL1? The 3-sigma upper confidence limit on the count-rate in the 0.3-1 keV band (UL_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableFUL2? The 3-sigma upper confidence limit on the count-rate in the 1-2 keV band (UL_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableFUL3? The 3-sigma upper confidence limit on the count-rate in the 2-10 keV band (UL_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullablePCR0? The peak count-rate in 0.3-10 keV band (PeakRate_band0)ct/sphot.count;arith.rate;em.X-raydoublenullableE_PCR0? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-10 keV band (PeakRate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_PCR0[]? The 1-sigma negative uncertainty on the peak count-rate in 0.3-10 keV band (PeakRate_band0_neg)ct/sstat.errordoublenullablePCR1? The peak count-rate in 0.3-1 keV band (PeakRate_band1)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_PCR1? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-1 keV band (PeakRate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_PCR1[]? The 1-sigma negative uncertainty on the peak count-rate in 0.3-1 keV band (PeakRate_band1_neg)ct/sstat.errordoublenullablePCR2? The peak count-rate in the 1-2 keV band (PeakRate_band2)ct/sphot.count;arith.rate;em.X-ray.softdoublenullableE_PCR2? The 1-sigma positive uncertainty on the peak count-rate in the 1-2 keV band (PeakRate_band2_pos)ct/sstat.error;stat.maxdoublenullablee_PCR2[]? The 1-sigma negative uncertainty on the peak count-rate in the 1-2 keV band (PeakRate_band2_neg)ct/sstat.errordoublenullablePCR3? The peak count-rate in the 2-10 keV band (PeakRate_band3)ct/sphot.count;arith.rate;em.X-ray.mediumdoublenullableE_PCR3? The 1-sigma positive uncertainty on the peak count-rate in the 2-10 keV band (PeakRate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_PCR3[]? The 1-sigma negative uncertainty on the peak count-rate in 2-10 keV band (PeakRate_band3_neg)ct/sstat.errordoublenullablePcstS0? The probability that the source count-rate in the 0.3-10 keV band does not vary between snapshots (PvarPchiSnapshot_band0)stat.fit.goodnessdoublenullablePcstS1? The probability that the source count-rate in the 0.3-1 keV band does not vary between snapshots (PvarPchiSnapshot_band1)stat.fit.goodnessdoublenullablePcstS2? The probability that the source count-rate in the 1-2 keV band does not vary between snapshots (PvarPchiSnapshot_band2)stat.fit.goodnessdoublenullablePcstS3? The probability that the source count-rate in the 2-10 keV band does not vary between snapshots (PvarPchiSnapshot_band3)stat.fit.goodnessdoublenullablePcstSHR1? The probability that the source HR1 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR1)stat.fit.goodnessdoublenullablePcstSHR2? The probability that the source HR2 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR2)stat.fit.goodnessdoublenullablePcst0? The probability that the source count-rate in the 0.3-10 keV band does not vary between observations (PvarPchiObsID_band0)stat.fit.goodnessdoublenullablePcst1? The probability that the source count-rate in the 0.3-1 keV band does not vary between observations (PvarPchiObsID_band1)stat.fit.goodnessdoublenullablePcst2? The probability that the source count-rate in the 1-2 keV band does not vary between observations (PvarPchiObsID_band2)stat.fit.goodnessdoublenullablePcst3? The probability that the source count-rate in the 2-10 keV band does not vary between observations (PvarPchiObsID_band3)stat.fit.goodnessdoublenullablePcstHR1? The probability that the source HR1 hardness ratio does not vary between observations (PvarPchiObsID_HR1)stat.fit.goodnessdoublenullablePcstHR2? The probability that the source HR2 hardness ratio does not vary between observations (PvarPchiObsID_HR2)stat.fit.goodnessdoublenullableNHgThe Galactic absorption column density (in cm-2) in the direction of the source, determined from Willingale et al (2013MNRAS.431..394W) (GalacticNH)cm**-2physdoublePow? Which of the available estimates of the power-law spectral ECF and fluxes (WhichPow) (6)meta.codeintnullableAPEC? Which of the available estimates of the APEC spectral ECF and fluxes (WhichAPEC) (7)meta.codeintnullableCFO0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming a power-law spectrum (PowECFO)mJ.m**-2.count**-1instr.paramdoublenullableCFU0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming a power-law spectrum (PowECFU)mJ.m**-2.count**-1instr.paramdoublenullableFPO0? The mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux_neg)mW.m**-2stat.errordoublenullableFPU0? The mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullablee_FPU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_neg)mW.m**-2stat.errordoublenullableECFO0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming an APEC spectrum (APECECFO)mJ.m**-2.count**-1instr.paramdoublenullableECFU0? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming an APEC spectrum (APECECFU)mJ.m**-2.count**-1instr.paramdoublenullableFAO0? The mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux_neg)mW.m**-2stat.errordoublenullableFAU0? The mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_neg)mW.m**-2stat.errordoublenullableFpPO0? The peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpPO0? The 1-sigma positive uncertainty on the peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpPO0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux_neg)mW.m**-2stat.errordoublenullableFpPU0? The peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpPU0? The 1-sigma positive uncertainty on the peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpPU0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_neg)mW.m**-2stat.errordoublenullableFpAO0? The peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpAO0? The 1-sigma positive uncertainty on the peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpAO0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux_neg)mW.m**-2stat.errordoublenullableFpAU0? The peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpAU0? The 1-sigma positive uncertainty on the peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpAU0[]? The 1-sigma negative uncertainty on the peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_neg)mW.m**-2stat.errordoublenullableCECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the canned power-law spectrum (FixedPowECFO)mJ.m**-2.count**-1instr.paramdoublenullableCECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the canned power-law spectrum (FixedPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableFCOP0? The mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCOP0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCOP0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux_neg)mW.m**-2stat.errordoublenullableFCUP0? The mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCUP0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCUP0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableAECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the canned APEC spectrum (FixedAPECECFO)mJ.m**-2.count**-1instr.paramdoublenullableAECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the canned APEC spectrum (FixedAPECECFU)mJ.m**-2.count**-1instr.paramdoublenullableFCAO0? The mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCAO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCAO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_neg)mW.m**-2stat.errordoublenullableFCAU0? The mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCAU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCAU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullablePECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFO)mJ.m**-2.count**-1instr.paramdoublenullablePECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableNH1H? The hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH)cm**-2phys.columnDensitydoublenullableE_NH1H[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH1H[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH_neg)cm**-2stat.errordoublenullableGam? The spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma)spect.indexdoublenullablee_Gam[]? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_neg)stat.errordoublenullableFIPO0? The mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_neg)mW.m**-2stat.errordoublenullableFIPU0? The mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableIPECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFO)mJ.m**-2.count**-1instr.paramdoublenullableIPECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFU)mJ.m**-2.count**-1instr.paramdoublenullableNH2A? The hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH)cm**-2phys.columnDensitydoublenullableE_NH2A[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2A[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_neg)cm**-2stat.errordoublenullablekTAH? The temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT)keVphys.temperaturedoublenullableE_kTAH[]? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT_pos)keVstat.error;stat.maxdoublenullablee_kTAH[]? The 1-sigma negative uncertainty on the temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT_neg)keVstat.errordoublenullableFAIO0? The mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAIO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAIO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_neg)mW.m**-2stat.errordoublenullableFAIU0? The mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullablee_FAIU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullablePpow? The probability that the HR values of this source could be obtained if the true spectrum is an absorbed power-law (P_pow)stat.fit.goodnessfloatnullablePAPEC? The probability that the HR values of this source could be obtained if the true spectrum is an APEC (P_APEC)stat.fit.goodnessfloatnullableFPECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFO)mJ.m**-2.count**-1instr.paramdoublenullableFPECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFU)mJ.m**-2.count**-1instr.paramdoublenullableNH2C? The hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH)cm**-2phys.columnDensitydoublenullableE_NH2C[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2C[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_neg)cm**-2stat.errordoublenullableGamma? The spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma)spect.indexdoublenullableE_Gamma[]? The 1-sigma positive uncertainty on the spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma_pos)stat.error;stat.maxdoublenullablee_Gamma[]? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma_neg)stat.errordoublenullableFPCO0? The mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPCO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPCO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_neg)mW.m**-2stat.errordoublenullableFPCU0? The mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPCU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPCU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableCstat? The C-statistic from the power-law spectral fit to the custom-built spectrum (FittedPowCstat)stat.fit.paramfloatnullableDOF? The number of degrees of freedom in the power-law spectral fit to the custom-built spectrum (FittedPowDOF)meta.numberintnullableChi2r? The Churazov-weighted reduced chi^2 from the power-law spectral fit to the custom-built spectrum (FittedPowReducedChi2)stat.fit.chi2floatnullableACECFO? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFO)mJ.m**-2.count**-1stat.fit.goodnessdoublenullableACECFU? The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFU)mJ.m**-2.count**-1stat.fit.goodnessdoublenullableNH2AC? The hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH)cm**-2phys.columnDensitydoublenullableE_NH2AC[]? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_pos)cm**-2stat.error;stat.maxdoublenullablee_NH2AC[]? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_neg)cm**-2stat.errordoublenullablekTAC? The temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT)keVphys.temperaturedoublenullableE_kTAC[]? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_pos)keVstat.error;stat.maxdoublenullablee_kTAC[]? The 1-sigma negative uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_neg)keVstat.errordoublenullableFACO0? The mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FACO0? The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FACO0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_neg)mW.m**-2stat.errordoublenullableFACU0? The mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FACU0? The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FACU0[]? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_neg)mW.m**-2stat.errordoublenullableCstatA? The C-statistic from the APEC spectral fit to the custom-built spectrum (FittedAPECCstat)stat.fit.paramdoublenullableDOFA? The number of degrees of freedom in the APEC spectral fit to the custom-built spectrum (FittedAPECDOF)meta.numberintnullableChi2rA? The Churazov-weighted reduced chi^2 from the APEC spectral fit to the custom-built spectrum (FittedAPECReducedChi2)stat.fit.chi2floatnullableHasSpecWhether a custom-built spectrum was created for this source (HasSpec)meta.codeintNExt? The number of external sources found to agree spatially with this one at the 3-sigma level (NumExternalMatches)meta.codeintnullableNExt2? The number of external sources found to agree spatially with this one at the 3-sigma level, excluding 2MASS and USNO-B1 matches (NumExternalMatches_slim)meta.codeintnullableROSHRIWhether the source is spatially within 3 sigma of a source in the Rosat HRI catalogue (Cat. IX/28) (MatchInROSHRI)meta.codeint2RXSWhether the source is spatially within 3 sigma of a source in the 2RXS catalogue (Cat. J/A+A/588/A103) (MatchIn2RXS)meta.codeint3XMMDR8Whether the source is spatially within 3 sigma of a source in the 3XMM-DR8 catalogue (Cat. IX/55) (MatchIn4XMM_DR10)meta.codeint3XMMDR7sWhether the source is spatially within 3 sigma of a source in the 3XMM-DR7s (stacked) catalogue (Cat. IX/56) (MatchIn4XMM_DR10s)meta.codeintXMMSL2Whether the source is spatially within 3 sigma of a source in the XMMSL2 catalogue (Cat. IX/53) (MatchInXMMSL2)meta.codeintSwiftFTWhether the source is spatially within 3 sigma of a source in the SwiftFT catalog (Cat. J/A+A/528/A122) (MatchInSwiftFT)meta.codeint1SWXRTWhether the source is spatially within 3 sigma of a source in the 1SWXRT catalogue (Cat. J/A+A/551/A142) (MatchIn1SWXRT)meta.codeintXRTGRBWhether the source is spatially within 3 sigma of an XRT GRB afterglow (MatchInXRTGRB)meta.codeintSDSSQSOWhether the source is spatially within 3 sigma of a source in the SDSS QSO DR14 catalogue (MatchInSDSS_QSO_DR14)meta.codeint2MASSWhether the source is spatially within 3 sigma of a source in the 2MASS catalogue (Cat. II/246) (MatchIn2MASS)meta.codeintUSNOB1Whether the source is spatially within 3 sigma of a source in the USNO-B1 catalogue (Cat. I/284) (MatchInUSNOB1)meta.codeint2CSCWhether the source is spatially within 3 sigma of a source in the 2CSC catalogue (MatchIn2CSC)meta.codeint2SXPSWhether the source is spatially within 3 sigma of a source in the 2SXPS (Cat. IX/58) catalogue (MatchIn2SXPS)meta.codeintAdDateThe date at which this source was added to LSXPS (WhenAdded)stime.epochnullableindexed
J/MNRAS/518/174/datasetsInformation about every individual datasets, observations and stacked images in LSXPSExpThe nominal exposure in the dataset, after all screening has been carried out (ExposureUsed)smeta.dataset;obs.exposuredoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDataIDThe unique identifier for this dataset (DatasetID)meta.idintObsIDThe identifier of the observation or stacked image in which this detection occurred (ObsID)meta.id;meta.mainVersionThe version of this dataset (DataVersion) (1)meta.version;meta.datasetintStackedWhether or not this is a stacked image (IsStackedImage)meta.codeintFFlagThe warning flag associated with this dataset (FieldFlag) (2)meta.codeintRAJ2000The right ascension of the field centre (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000The declination of the field centre (J2000) (Decl)degpos.eq.dec;meta.mainindexedGLONGalactic longitude of the field centre (l)degpos.galactic.lonGLATGalactic latitude of the field centre (b)degpos.galactic.latdoubleSizeThe side length of the field image in XRT pixels (2.357 arcsec per pixel) (ImageSize)phys.size;obs.fieldintt.start1The UTC start time of the dataset (StartTime_UTC)stime.epochnullablet.stop1The UTC end time of the dataset (StopTime_UTC)stime.epochnullableOExpThe original nominal exposure in the dataset before screening (OriginalExposure)smeta.dataset;obs.exposuredoubletime.start1The start time of the dataset, in Swift Mission Elapsed Time (StartTime_MET)stime.epochlongtime.stop1The end time of the dataset, in Swift Mission Elapsed Time (StopTime_MET)stime.epochlongtime.mid1The mid-time of the dataset, in Swift Mission Elapsed Time (MidTime_MET)stime.epochlongtime.mid2The mid-time of the dataset, in Barycentric Dynamical Time (MidTime_TDB)stime.epochdoubletime.mid3The mid-time of the dataset, as a Modified Julian Date (MidTime_MJD)stime.epochdoubleLiveDateThe UTC date at which this dataset became live (LiveDate)stime.epochnullableindexedFBGb0The mean background level in the 0.3-10 keV band (FieldBG_band0)count.pixel**-1.s**-1instr.background;em.X-ray.medium;stat.meandoubleFBGb1The mean background level in the 0.3-1 keV band (FieldBG_band1)count.pixel**-1.s**-1instr.background;em.X-ray.soft;stat.meandoubleFBGb2The mean background level in the 1-2 keV band (FieldBG_band2)count.pixel**-1.s**-1instr.background;em.X-ray.soft;stat.meandoubleFBGb3The mean background level in the 2-10 keV band (FieldBG_band3)count.pixel**-1.s**-1instr.background;em.X-ray.medium;stat.meandoubleNbr0The number of sources detected in this dataset in the 0.3-10 keV band (NumSrc_band0)meta.numberintNOK0The number of good or reasonable sources detected in this dataset in the 0.3-10 keV band (NumOK_band0)meta.numberintMD0? The median distance between sources detected in this dataset in the 0.3-10 keV band (MedianDist_band0)pcpos.distancefloatnullableNbr1The number of sources detected in this dataset in the 0.3-1 keV band (NumSrc_band1)meta.numberintNOK1The number of good or reasonable sources detected in this dataset in the 0.3-1 keV band (NumOK_band1)meta.numberintMD1? The median distance between sources detected in this dataset in the 0.3-1 keV band (MedianDist_band1)pcpos.distancefloatnullableNbr2The number of sources detected in this dataset in the 1-2 keV band (NumSrc_band2)meta.numberintNOK2The number of good or reasonable sources detected in this dataset in the 1-2 keV band (NumOK_band2)meta.numberintMD2? The median distance between sources detected in this dataset in the 1-2 keV band (MedianDist_band2)pcpos.distancefloatnullableNbr3The number of sources detected in this dataset in the 2-10 keV band (NumSrc_band3)meta.numberintNOK3The number of good or reasonable sources detected in this dataset in the 2-10 keV band (NumOK_band3)meta.numberintMD3? The median distance between sources detected in this dataset in the 2-10 keV band (MedianDist_band3)pcpos.distancefloatnullableNSnapsThe number of snapshots contributing to this dataset (NumberOfSnapshots)meta.numberintErrAst? The 90% confidence radial uncertainty on the XRT-2MASS astrometric correction (AstromError)arcsecstat.errorfloatnullableCRV1c? The CRVAL1 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CRVAL1_corr)instr.paramdoublenullableCRV2c? The CRVAL2 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CRVAL2_corr)instr.paramdoublenullableCROT2c? The CROTA1 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CROTA2_corr)instr.paramdoublenullableStackWhether this corresponds to a stacked image which has been superseded by a newer version, but which contains a unique detection of a source (IsObsoleteStack)meta.codeint
J/MNRAS/518/174/dcleanSubset of datasets.dat where FFlag=0 or 1time.mid3The mid-time of the dataset, as a Modified Julian Date (MidTime_MJD)stime.epochdoubleLiveDateThe UTC date at which this dataset became live (LiveDate)stime.epochnullableindexedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDataIDThe unique identifier for this dataset (DatasetID)meta.idintObsIDThe identifier of the observation or stacked image in which this detection occurred (ObsID)meta.id;meta.mainVersionThe version of this dataset (DataVersion) (1)meta.version;meta.datasetintStackedWhether or not this is a stacked image (IsStackedImage)meta.codeintFFlagThe warning flag associated with this dataset (FieldFlag) (2)meta.codeintRAJ2000The right ascension of the field centre (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000The declination of the field centre (J2000) (Decl)degpos.eq.dec;meta.mainindexedGLONGalactic longitude of the field centre (l)degpos.galactic.lonGLATGalactic latitude of the field centre (b)degpos.galactic.latdoubleSizeThe side length of the field image in XRT pixels (2.357 arcsec per pixel) (ImageSize)phys.size;obs.fieldintExpThe nominal exposure in the dataset, after all screening has been carried out (ExposureUsed)smeta.dataset;obs.exposuredoublet.start1The UTC start time of the dataset (StartTime_UTC)stime.epochnullablet.stop1The UTC end time of the dataset (StopTime_UTC)stime.epochnullableOExpThe original nominal exposure in the dataset before screening (OriginalExposure)smeta.dataset;obs.exposuredoubletime.start1The start time of the dataset, in Swift Mission Elapsed Time (StartTime_MET)stime.epochlongtime.stop1The end time of the dataset, in Swift Mission Elapsed Time (StopTime_MET)stime.epochlongtime.mid1The mid-time of the dataset, in Swift Mission Elapsed Time (MidTime_MET)stime.epochlongtime.mid2The mid-time of the dataset, in Barycentric Dynamical Time (MidTime_TDB)stime.epochdoubleFBGb0The mean background level in the 0.3-10 keV band (FieldBG_band0)count.pixel**-1.s**-1instr.background;em.X-ray.medium;stat.meandoubleFBGb1The mean background level in the 0.3-1 keV band (FieldBG_band1)count.pixel**-1.s**-1instr.background;em.X-ray.soft;stat.meandoubleFBGb2The mean background level in the 1-2 keV band (FieldBG_band2)count.pixel**-1.s**-1instr.background;em.X-ray.soft;stat.meandoubleFBGb3The mean background level in the 2-10 keV band (FieldBG_band3)count.pixel**-1.s**-1instr.background;em.X-ray.medium;stat.meandoubleNbr0The number of sources detected in this dataset in the 0.3-10 keV band (NumSrc_band0)meta.numberintNOK0The number of good or reasonable sources detected in this dataset in the 0.3-10 keV band (NumOK_band0)meta.numberintMD0? The median distance between sources detected in this dataset in the 0.3-10 keV band (MedianDist_band0)pcpos.distancefloatnullableNbr1The number of sources detected in this dataset in the 0.3-1 keV band (NumSrc_band1)meta.numberintNOK1The number of good or reasonable sources detected in this dataset in the 0.3-1 keV band (NumOK_band1)meta.numberintMD1? The median distance between sources detected in this dataset in the 0.3-1 keV band (MedianDist_band1)pcpos.distancefloatnullableNbr2The number of sources detected in this dataset in the 1-2 keV band (NumSrc_band2)meta.numberintNOK2The number of good or reasonable sources detected in this dataset in the 1-2 keV band (NumOK_band2)meta.numberintMD2? The median distance between sources detected in this dataset in the 1-2 keV band (MedianDist_band2)pcpos.distancefloatnullableNbr3The number of sources detected in this dataset in the 2-10 keV band (NumSrc_band3)meta.numberintNOK3The number of good or reasonable sources detected in this dataset in the 2-10 keV band (NumOK_band3)meta.numberintMD3? The median distance between sources detected in this dataset in the 2-10 keV band (MedianDist_band3)pcpos.distancefloatnullableNSnapsThe number of snapshots contributing to this dataset (NumberOfSnapshots)meta.numberintErrAst? The 90% confidence radial uncertainty on the XRT-2MASS astrometric correction (AstromError)arcsecstat.errorfloatnullableCRV1c? The CRVAL1 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CRVAL1_corr)instr.paramdoublenullableCRV2c? The CRVAL2 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CRVAL2_corr)instr.paramdoublenullableCROT2c? The CROTA1 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CROTA2_corr)instr.paramdoublenullableStackWhether this corresponds to a stacked image which has been superseded by a newer version, but which contains a unique detection of a source (IsObsoleteStack)meta.codeint
J/MNRAS/518/174/ducleanSubset of dclean where FFlag=0StackedWhether or not this is a stacked image (IsStackedImage)meta.codeintFBGb3The mean background level in the 2-10 keV band (FieldBG_band3)count.pixel**-1.s**-1instr.background;em.X-ray.medium;stat.meandoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDataIDThe unique identifier for this dataset (DatasetID)meta.idintObsIDThe identifier of the observation or stacked image in which this detection occurred (ObsID)meta.id;meta.mainVersionThe version of this dataset (DataVersion) (1)meta.version;meta.datasetintFFlagThe warning flag associated with this dataset (FieldFlag) (2)meta.codeintRAJ2000The right ascension of the field centre (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000The declination of the field centre (J2000) (Decl)degpos.eq.dec;meta.mainindexedGLONGalactic longitude of the field centre (l)degpos.galactic.lonGLATGalactic latitude of the field centre (b)degpos.galactic.latdoubleSizeThe side length of the field image in XRT pixels (2.357 arcsec per pixel) (ImageSize)phys.size;obs.fieldintExpThe nominal exposure in the dataset, after all screening has been carried out (ExposureUsed)smeta.dataset;obs.exposuredoublet.start1The UTC start time of the dataset (StartTime_UTC)stime.epochnullablet.stop1The UTC end time of the dataset (StopTime_UTC)stime.epochnullableOExpThe original nominal exposure in the dataset before screening (OriginalExposure)smeta.dataset;obs.exposuredoubletime.start1The start time of the dataset, in Swift Mission Elapsed Time (StartTime_MET)stime.epochlongtime.stop1The end time of the dataset, in Swift Mission Elapsed Time (StopTime_MET)stime.epochlongtime.mid1The mid-time of the dataset, in Swift Mission Elapsed Time (MidTime_MET)stime.epochlongtime.mid2The mid-time of the dataset, in Barycentric Dynamical Time (MidTime_TDB)stime.epochdoubletime.mid3The mid-time of the dataset, as a Modified Julian Date (MidTime_MJD)stime.epochdoubleFBGb0The mean background level in the 0.3-10 keV band (FieldBG_band0)count.pixel**-1.s**-1instr.background;em.X-ray.medium;stat.meandoubleFBGb1The mean background level in the 0.3-1 keV band (FieldBG_band1)count.pixel**-1.s**-1instr.background;em.X-ray.soft;stat.meandoubleFBGb2The mean background level in the 1-2 keV band (FieldBG_band2)count.pixel**-1.s**-1instr.background;em.X-ray.soft;stat.meandoubleNbr0The number of sources detected in this dataset in the 0.3-10 keV band (NumSrc_band0)meta.numberintNOK0The number of good or reasonable sources detected in this dataset in the 0.3-10 keV band (NumOK_band0)meta.numberintMD0? The median distance between sources detected in this dataset in the 0.3-10 keV band (MedianDist_band0)pcpos.distancefloatnullableNbr1The number of sources detected in this dataset in the 0.3-1 keV band (NumSrc_band1)meta.numberintNOK1The number of good or reasonable sources detected in this dataset in the 0.3-1 keV band (NumOK_band1)meta.numberintMD1? The median distance between sources detected in this dataset in the 0.3-1 keV band (MedianDist_band1)pcpos.distancefloatnullableNbr2The number of sources detected in this dataset in the 1-2 keV band (NumSrc_band2)meta.numberintNOK2The number of good or reasonable sources detected in this dataset in the 1-2 keV band (NumOK_band2)meta.numberintMD2? The median distance between sources detected in this dataset in the 1-2 keV band (MedianDist_band2)pcpos.distancefloatnullableNbr3The number of sources detected in this dataset in the 2-10 keV band (NumSrc_band3)meta.numberintNOK3The number of good or reasonable sources detected in this dataset in the 2-10 keV band (NumOK_band3)meta.numberintMD3? The median distance between sources detected in this dataset in the 2-10 keV band (MedianDist_band3)pcpos.distancefloatnullableNSnapsThe number of snapshots contributing to this dataset (NumberOfSnapshots)meta.numberintErrAst? The 90% confidence radial uncertainty on the XRT-2MASS astrometric correction (AstromError)arcsecstat.errorfloatnullableCRV1c? The CRVAL1 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CRVAL1_corr)instr.paramdoublenullableCRV2c? The CRVAL2 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CRVAL2_corr)instr.paramdoublenullableCROT2c? The CROTA1 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CROTA2_corr)instr.paramdoublenullableStackWhether this corresponds to a stacked image which has been superseded by a newer version, but which contains a unique detection of a source (IsObsoleteStack)meta.codeintLiveDateThe UTC date at which this dataset became live (LiveDate)stime.epochnullableindexed
J/MNRAS/518/174/detect*Specific individual X-ray detections catalog in all band before combination to create sourcesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDetIDA unique identifier for this detection (DetectionID)meta.id;meta.mainintDataIDThe unique identifier for the dataset in which the detection occurred (DatasetID)meta.idintObsIDThe obsID of the observation in which the detection occurred (ObsID)meta.id;obsObsSIDThe ID of the obsSource this detection is part of (ObsSourceID)meta.idintprimaryLSXPS? The ID of the LSXPS source of which this is a detection (LSXPS_ID)meta.idintnullableSNoThe identifier of this source within this obsid and band (SourceNo)meta.idintBandThe band in which this detection occurred (Band) (1)instr.bandpassintExpCorThe exposure time at the position of the source in this obsID (CorrectedExposure)stime.duration;obs.exposuredoubleExpFracThe fractional exposure at the position of this source, i.e. the exposure divided by the nominal exposure for the field (ExposureFraction)stime.expofloatOffAxisThe angular distance of the source from the XRT boresight in all observations within which the source was detected (OffaxisAngle)arcminpos.angDistancefloatRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedE_RAJ2000The 1-sigma positive uncertainty on the right ascension (RA_pos)degstat.error;stat.maxdoublee_RAJ2000The 1-sigma negative uncertainty on the right ascension (RA_neg)degstat.error;pos.eq.radoubleDEJ2000Declination (J2000) (Decl)degpos.eq.dec;meta.mainindexedE_DEJ2000The 1-sigma positive uncertainty on the declination (Decl_pos)degstat.error;stat.maxdoublee_DEJ2000The 1-sigma negative uncertainty on the declination (Decl_neg)degstat.error;pos.eq.decdoubleErr90Position uncertainty, 90% confidence, radial, assumed to be Rayleigh-distributed (Err90)arcsecstat.errorfloatRAcordeg? Right Ascension corrected using XRT-2MASS astrometry (J2000) (RA_corrected)degpos.eq.ranullableDEcordeg? Declination corrected using XRT-2MASS astrometry (J2000) (Decl_corrected)degpos.eq.decnullableErr90corr? Uncertainty on the corrected position, 90% confidence, radial, assumed to be Rayleigh-distributed (Err90_corrected)arcsecstat.error;posfloatnullableGLONGalactic longitude (l)degpos.galactic.lonGLATGalactic latitude (b)degpos.galactic.latdoubleGLONcor? Galactic longitude corrected using XRT-2MASS astrometry (l_corrected)degpos.galactic.lonnullableGLATcor? Galactic latitude corrected using XRT-2MASS astrometry (b_corrected)degpos.galactic.latdoublenullableXThe x position of the object in the SKY image plane (IMG_X)pixpos.cartesian.x;instr.platedoubleYThe y position of the object in the SKY image plane (IMG_Y)pixpos.cartesian.y;instr.platedoubleDNNThe distance to the closest detection to this one, in this image (NearestNeighbour)arcsecpos.angDistancefloatDNNOKThe distance to the closest Good or reasonable detection to this one, in this image (NearestOKNeighbour)arcsecpos.angDistancefloatDetFlagThe best detection flag from all detections of the source (DetFlag) (2)meta.codeintWarningWhether this detection is potentially affected by optical loading (OpticalLoadingWarning) (3)magphot.mag;em.optdoubleDetSLWWhether this detection occurred within fitted stray light rings (StrayLightWarning)meta.codeintDetNBSWWhether this detection occurred within the PSF wings of a fitted bright source (NearBrightSourceWarning)meta.codeintMatchXWhether the position of this source matches a known extended X-ray source (MatchesKnownExtended)meta.codeintPileupWhether the accepted fit included pile up (PileupFitted)meta.codeintSNRThe signal to noise ratio of the detection (SNR)stat.snrfloatCtsPSFNumber of counts in the image region over which the final PSF fit was performed (CtsInPSFFit)ctphot.count;em.X-rayintBGPSFMean count-rate in the background map in the region over which the final PSF fit was performed (BGRateInPSFFit)ct/sphot.count;em.X-raydoubleCstatThe C-statistic value from the PSF fit (Cstat)stat.fit.paramdoubleCstatNoThe C-statistic value derived over the PSF fit region if no source is fitted (Cstat_nosrc)stat.fit.paramdoubleLsrcThe log-likelihood value that this detection is not just a background fluctuation (L_src)stat.likelihoodfloatCstatFThe Cstat value found from a fit assuming a constant increase above the background (i.e. the count excess is flat, not PSFlike) (Cstat_flat)stat.fit.paramdoubleLFlatThe log-likelihood value that this detection is PSF like, not a flat count increase (Lflat)stat.likelihoodfloatFracPixThe fraction of pixels within the PSF fit region which are exposed (FracPix)instr.saturationfloatPileSThe best-fitting S parameter of the pile-up model, if fitted (Pileup_S)stat.fit.paramfloatPilelThe best-fitting l parameter of the pile-up model, if fitted (Pileup_l)stat.fit.paramfloatPilecThe best-fitting c parameter of the pile-up model, if fitted (Pileup_c)stat.fit.paramfloatPiletauThe best-fitting tau parameter of the pile-up model, if fitted (Pileup_tau)stat.fit.paramfloatCstatPileThe Cstat value found from the unusued fit i.e. if the piled up model was used, this gives the Cstat from the non-piled-up fit, and vice-versa (Cstat_altPileup)stat.fit.paramdoublePSFRadThe radius of the circular region over which PSF fitting was carried out (in image pixels, 2.357"" to a side) (PSF_Fit_Radius)instr.det.psf;obs.fieldintBoxWidthThe full width of the cell-detect box in which this source was detected (in image pixels, 2.357"" to a side) (CellDetect_BoxWidth)spect.line.widthintRateThe corrected count-rate of this detection (i.e. in the band of this image) (Rate)ct/sphot.count;em.X-raydoubleE_RateThe 1-sigma positive uncertainty on the count rate (Rate_pos)ct/sstat.error;stat.maxdoublee_RateThe 1-sigma negative uncertainty on the count rate (Rate_neg)ct/sstat.errordoubleCtsThe total number of counts in the region used to extract the count rate (CtsInRate)ctphot.count;em.X-rayintBGCtsThe total number of counts in the region used to extract the count rate (BGCtsInRate)ctphot.count;em.X-raydoubleCFThe PSF correction factor for the count rate (Rate_CF)instr.paramdoubleBGRateThe background rate in the region used for count-rate calculation (BGRateInRate)ct/sphot.count;em.X-raydoubleObsLink to obsourcemeta.ref.urlchar
J/MNRAS/518/174/obsource*Details of the detections in an individual dataset, merged over all bandse_HR1? The 1-sigma negative uncertainty on the aggregate HR1 hardness ratio of the obsSource (HR1_neg)stat.errordoublenullableHR2? The aggregate HR2 hardness ratio of the obsSource (HR2)phot.flux;arith.ratiofloatnullableE_HR2? The 1-sigma positive uncertainty on the aggregate HR2 hardness ratio of the obsSource (HR2_pos)stat.error;stat.maxdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObsSIDThe unique identifier of this ObsSource (ObsSourceID)meta.id;meta.mainDataIDThe dataset identifier in which this obsSource was found (DatasetID)meta.idintLSXPS? Numerical unique source identifier within LSXPS (LSXPS_ID) ?meta.idintnullableOSNumThe identifier of this obsSource within this dataset (OSNum)meta.idintCorPosWhether or not the astrometrically-corrected position of this obsSource should be used (UsedCorrectedPosition)meta.codeintDNN? The distance (in arcseconds) to the closest LSXPS obsSource within this dataset (NearestNeighbour)arcsecpos.angDistancefloatnullableDNNOK? The distance (in arcseconds) to the closest good or reasonable LSXPS obsSource within this dataset (NearestOKNeighbour)arcsecpos.angDistancefloatnullableExpThe exposure time at the position of the obsSource, corrected for vignetting (Exposure)stime.duration;obs.exposureintHR1? The aggregate HR1 hardness ratio of the obsSource (HR1)phot.flux;arith.ratiofloatnullableE_HR1? The 1-sigma positive uncertainty on the aggregate HR1 hardness ratio of the obsSource (HR1_pos)stat.error;stat.maxdoublenullablee_HR2? HR2_neg The 1-sigma negative uncertainty on the aggregate HR2 hardness ratio of the obsSource (HR2_neg)stat.errordoublenullableBBandThe energy band corresponding to the best detection of this obsSource in this dataset (BestBand)instr.bandpassintPile? Whether a pileup warning exists, indicating that the object is very piled up and in some bands there is evidence of pile up not being fitted (PileupWarning)meta.codeintnullableDetIDThe DetectionID of the best detection of this obsSource in this dataset (BestDetectionID)meta.id.associntOrphanWhether this source is one which is only detected in this dataset, and this dataset is deprecated (IsOrphanSource)meta.codeint
J/MNRAS/518/174/xcorrDetails of the cross correlation between the LSXPS sources and other cataloguesLSXPSThe numerical identifier of the LSXPS source (LSXPS_ID)meta.id;meta.mainintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintExtCatThe catalogued name of the external source (ExtCat_ID)meta.id.assoccharCatThe catalogue in which the external source was found (Catalogue)meta.id;meta.datasetcharDThe distance between the 2SXPS and external source positions (Distance)arcsecpos.angDistancefloatExtRAThe right ascension of the external source (J2000) (Ext_RA)degpos.eq.ra;meta.mainExtDEThe declination of the external source (J2000) (Ext_Decl)degpos.eq.dec;meta.mainExtErr90? The 90% confidence radial position error of the external source (Ext_Err90) (1)arcsecstat.errorfloatnullable
J/MNRAS/518/174/oldstackDetails of the stacked images which have been superseded by newer datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDataIDThe unique identifier for this dataset (DatasetID)meta.id;meta.mainintDataVThe version of this dataset (DataVersion) (1)meta.softwareintLiveDateThe UTC date at which this dataset became live (LiveDate)stime.epochnullableindexedObsIDThe identifier of the observation or stacked image in which this detection occurred (ObsID)meta.id;obs.param;obsObsoleteWhether this corresponds to a stacked image which has been superseded by a newer version, but which contains a unique detection of a source (IsObsoleteStack)meta.codeint
J/MNRAS/518/174/transTransient counterpart checked by the XRT team and classed into 'possible transient' categoriesDEJ2000Declination (J2000) (Decl)degpos.eq.dec;meta.mainErr90Position uncertainty, 90% confidence, radial, assumed to be Rayleigh-distributed (Err90)arcsecstat.errorfloatGLONGalactic longitude (l)degpos.galactic.lonGLATGalactic latitude (b)degpos.galactic.latdoubleDofFS? The number of degrees of freedom in the automated power-law fit to a spectrum built from the all observations of the transient after its discovery (FullSpecDof)meta.numberintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTrsIDA unique numerical identifier for this transient within this catalogue (TransientID)meta.id;meta.mainintIAUNameThe IAU-format name of the transient: SwiftJ HHMMSS.S+ddmmss (IAUName)meta.idcharLSXPS? The source identifier within the main LSXPS catalogue (LSXPS_ID)meta.idintnullableLSXPSNThe IAU name of this object in the main LSXPS catalogue (LSXPSName)meta.idcharClassA numerical code describing how this transient has been classified e.g 64 cases of 1 as confirmed transient (Classification)meta.codeintRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainDiscoveryThe date of the observation in ident number in which the transient was first found (DiscoveryDatasetID)meta.numberintObsSIDThe numerical identified of the first detection in the Public_ObsSources table (ObsSourceID)meta.idintPRateThe peak count-rate in the 0.3-10 keV band in the dataset in which the transient was first detected (PeakRateAtDetection)ct/sphot.count;em.X-raydoubleE_PRateThe 1-sigma positive uncertainty on the peak count-rate in the 0.3-10 keV band in the dataset in which the transient was first detected (PeakRateAtDetection_pos)ct/sstat.error;stat.maxdoublee_PRateThe 1-sigma negative uncertainty on the peak count-rate in the 0.3-10 keV band in the dataset in which the transient was first detected (PeakRateAtDetection_neg)ct/sstat.errordoublePSMRateThe peak count-rate in the 0.3-2 keV band in the dataset in which the transient was first detected (PeakSoftMedBandRateAtDetection)ct/sphot.count;em.X-ray.softdoubleUpperDSWhere the 'best' upper limit at the source location was taken from, where the discovery spectrum is used to convert between observatories (UpperLimitSource_DS)meta.notecharUpperFSWhere the 'best' upper limit at the source location was taken from, where the full spectrum is used to convert between observatories (UpperLimitSource_FS)meta.notecharSigHow far above the best upper limit the peak count rate is, in Gaussian sigmas (Significance)arith.rate;phot.count;stat.maxfloatNH? The hydrogen column density found in an automated power-law fit to a spectrum built from the discovery dataset (InitSpecNH)cm**-2phys.columnDensity;meta.modelleddoublenullableGamma? The photon index found in an automated power-law fit to a spectrum built from the discovery dataset (InitSpecGamma)meta.code;em.energy;meta.modelleddoublenullableCstat? The C-statistic from an automated power-law fit to a spectrum built from the discovery dataset. (InitSpecCstat)stat.fit.paramfloatnullableChi2? The Churazov-weighted reduced chi^2 from an automated power-law fit to a spectrum built from the discovery dataset (InitSpecTestStat)stat.fit.chi2floatnullableDof? The number of degrees of freedom in the automated power-law fit to a spectrum built from the discovery dataset (InitSpecDof)meta.numberintnullableNHFS? The hydrogen column density found in an automated power-law fit to a spectrum built from all observations of the transient after its discovery (FullSpecNH)cm**-2phys.columnDensity;meta.modelleddoublenullableGammaFS? The photon index found in an automated power-law fit to a spectrum built from all observations of the transient after its discovery (FullSpecGamma)spect.indexdoublenullableCstatFS? The C-statistic from an automated power-law fit to a spectrum built from all observations of the transient after its discovery (FullSpecCstat)stat.fit.paramfloatnullableChi2FS? The Churazov-weighted reduced chi^2 from an automated power-law fit to a spectrum built from all observations of the transient after its discovery (FullSpecTestStat)stat.fit.chi2floatnullableDiscDate? The date of the analysis in which the transient was first found (DiscoveryDate)stime.epochnullableDetDate? The date of the start of the observation in which the transient was first found (DetectionDate)yrtime.epochintnullableDetMETThe MET of the start of the observation in which the transient was first found (DetectionMET)stime.epochdoubleLSXPSul? An upper limit at the transient derived from the LSXPS catalogue (LSXPS_UpperLimit)ct/sphot.count;em.X-raydoublenullableLSXPSulID? The observation in the LSXPS catalogue from which the upper limit was derived (LSXPS_UpperLimit_ObsID)meta.numberdoublenullableXMMul? An XMM-Newton upper limit at the transient location, obtained via the HILIGT server, in native XMM count-rate units (XMM_UpperLimit_native)ct/sphot.count;em.X-raydoublenullableXMMulModeThe mode in which XMM was observing when the upper limit was obtained (XMM_UpperLimit_ObsMode)meta.codecharXMMulInstThe XMM-Newton instrument from which the upper limit was obtained (XMM_UpperLimit_Instrument)meta.codecharXMMulXRTds? The XMM-Newton upper limit converted to a 0.3-10 keV XRT count rate, using the automated power-law fit to a spec. built from the discovery dataset (XMM_UpperLimit_asXRTTotal_DS)ct/sphot.count;em.X-raydoublenullableXMMulXRTfs? The XMM-Newton upper limit converted to a 0.3-10 keV XRT count rate, using the automated power-law fit to a spect. built from the all obs. of the transient after its discovery (XMM_UL_asXRTTot_FS)ct/sphot.count;em.X-raydoublenullableXMMulXRTc? The XMM-Newton upper limit converted to a 0.3-10 keV XRT count rate, using a standard AGN spectrum (XMM_UpperLimit_asXRTTotal_Canned)ct/sphot.count;em.X-raydoublenullableRSulAn ROSAT All-Sky Survey upper limit at the transient location, obtained via the HILIGT server, in native ROSAT PSPC count-rate units (RASS_UpperLim_native)ct/sphot.count;em.X-raydoubleRSulXRTsmds? The RASS upper limit converted to a 0.3-2 keV XRT count rate, using the automated power-law fit to a spectrum built from the discovery dataset (RASS_UpperLimit_asXRTSoftMed_DS)ct/sphot.count;em.X-raydoublenullableRSulXRTsmfs? The RASS upper limit converted to a 0.3-2 keV XRT count rate, using the automated power-law fit to a spectrum built from the all observations of the transient after its discovery (RASS_UpperLimit_asXRTSoftMed_FS)ct/sphot.count;em.X-raydoublenullableRSulXRTsmcThe RASS upper limit converted to a 0.3-2 keV XRT count rate, using a standard AGN spectrum (RASS_UpperLimit_asXRTSoftMed_Canned)ct/sphot.count;em.X-raydoubleRSulXRTds? The RASS upper limit converted to a 0.3-10 keV XRT count rate, using the automated power-law fit to a spectrum built from the discovery dataset (RASS_UpperLimit_asXRTTotal _DS)ct/sphot.count;em.X-raydoublenullableRSulXRTfs? The RASS upper limit converted to a 0.3-10 keV XRT count rate, using the automated power-law fit to a spectrum built from the all observations of the transient after its discovery (RASS_UpperLimit_asXRTTotal_FS)ct/sphot.count;em.X-raydoublenullableRSulXRTc? The RASS upper limit converted to a 0.3-10 keV XRT count rate, using a standard AGN spectrum (RASS_UpperLimit_asXRTTotal_Canned)ct/sphot.count;em.X-raydoublenullableNotesAny notes added by the XRT team (Notes)meta.notecharUpperCWhere the 'best' upper limit at the source location was taken from, where the 'canned' spectrum is used to convert between observatories (UpperLimitSource_Canned)meta.notechar