IX/58/2sxpsThe 2SXPS Catalogue of Swift X-ray telescope Point SourcesE_CR2? The 1-sigma positive uncertainty on the mean count-rate in the 1-2keV band (Rate_band2_pos)ct/sstat.error;stat.maxdoublenullablekTAH? The temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT)keVspect.indexdoublenullableDOF? The number of degrees of freedom in the power-law spectral fit to the custom-built spectrum (FittedPowDOF)stat.fit.dofintnullableIAUNameIAU-format name, 2SXPS JHHMMSS+-ddmmsss (IAUName)meta.idcharE_FPU0The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_pos)mW.m**-2stat.error;stat.maxcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint2SXPSNumerical unique source identifier within 2SXPS (2SXPS_ID)meta.id;meta.mainintRAJ2000Right 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.errorfloatA[0/1] Provenance of source astrometry. 0=Swift star tracker, 1=XRT/2MASS astrometry (AstromType)meta.ref;pos.frameintGLONGalactic longitude (l)degpos.galactic.lonGLATGalactic latitude (b)degpos.galactic.latdoubleOffAxisThe mean angular distance of the source from the XRT boresight in all observations within which the source was detected (MeanOffAxisAngle) (1)arcminpos.angDistance;stat.meanfloatDNNThe distance to the closest 2SXPS source to this one (NearestNeighbour)arcsecpos.angDistancedoubleDNNOKThe distance to the closest 2SXPS source to this one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour)arcsecpos.angDistancedoublet.expThe total exposure at the source location in the catalogue (Exposure)stime.expointt.start1The UTC date & time of the start of the first observation in 2SXPS which covered the source location (FirstObsDate)stime.epochnullablet.stop1The UTC date & time of the end of the last observation in 2SXPS which covered the source location (LastObsDate)stime.epochnullabletime.start1The time of the start of the first observation in 2SXPS which covered the source location, in Swift Mission Elapsed Time (FirstObsMET) (2)stime.expolongtime.stop1The time of the end of the last observation in 2SXPS which covered the source location in, Swift Mission Elapsed Time (LastObsMET) (2)stime.expolongt.start2The UTC date & time of the start of the first observation in 2SXPS in which the source count rate is inconsistent with 0 at the 3-sigma level (FirstDetDate)stime.epochnullablet.stop2The UTC date & time of the end of the last observation in 2SXPS in which the source count rate is inconsistent with 0 at the 3-sigma level (LastDetDate)stime.epochnullabletime.start2The time of the start of the first observation in 2SXPS in which the source count rate is inconsistent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (FirstDetMET)(2)stime.expolongtime.stop2The time of the end of the last observation in 2SXPS in which the source count rate is inconsistent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (LastDetMET) (2)stime.expolongt.start3The UTC date & time of the start of the first observation in 2SXPS 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 2SXPS in which the source is detected in the blind search (LastBlindDetDate)stime.epochnullabletime.start3The time of the start of the first observation in 2SXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (FirstBlindDetMET) (2)stime.expolongtime.stop3The time of the end of the last observation in 2SXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (LastBlindDetMET) (2)stime.expolongNObsThe number of observations covering this source's position (NumObs)meta.numberintNBlindThe number of observations in which this source was found in a blind search (NumBlindDetObs)meta.numberintNDetThe number of observations in which this source is detected (NumDetObs)meta.numberintNBestThe ID of the 'best' detection (BestDetectionID)meta.numberintF0Whether the count-rate in the 0.3-10keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band0)meta.codeintF1Whether the count-rate in the 0.3-1keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band1)meta.codeintF2Whether the count-rate in the 1-2keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band2)meta.codeintF3Whether the count-rate in the 2-10keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band3)meta.codeintDet? The final source detection flag (DetFlag) (3)meta.code.error;phys.atmol.finalintnullableFField? The final fieldFlag for this source (FieldFlag) (4)meta.codeintnullableDet0? The final detection flag the 0.3-10keV band (DetFlag_band0) (3)meta.code.qualintnullableDet1? The final detection flag the 0.3-1keV band (DetFlag_band1) (3)meta.code.qualintnullableDet2? The final detection flag in the 1-2keV band (DetFlag_band2) (3)meta.code.qualintnullableDet3? The final detection flag in the 2-10keV band (DetFlag_band3) (3)meta.code.qualintnullableWarningThe worst optical loading warning from all detections of this source (5)magmeta.codedoubleDetSLWWhether 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.codeintCR0? The mean count-rate in the 0.3-10keV band (Rate_band0)ct/sphot.count;em.X-raydoublenullableE_CR0? The 1-sigma positive uncertainty on the mean count-rate in the 0.3-10keV band (Rate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_CR0[]? The 1-sigma negative uncertainty on the mean count-rate in the 0.3-10keV 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.maxfloatnullablee_HR1[]? The 1-sigma negative uncertainty on the aggregate HR1 hardness ratio of the source (HR1_neg)stat.errorfloatnullableHR2? 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.maxfloatnullablee_HR2[]? The 1-sigma negative uncertainty on the aggregate HR2 hardness ratio of the source (HR2_neg)stat.errorfloatnullableCR1? The mean count-rate in the 0.3-1keV band (Rate_band1)ct/sphot.count;em.X-raydoublenullableE_CR1? The 1-sigma positive uncertainty on the mean count-rate in the 0.3-1keV band (Rate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_CR1[]? The 1-sigma negative uncertainty on the mean count-rate in the 0.3-1keV band (Rate_band1_neg)ct/sstat.errordoublenullableCR2? The mean count-rate in the 1-2keV band (Rate_band2)ct/sphot.count;em.X-raydoublenullablee_CR2[]? The 1-sigma negative uncertainty on the mean count-rate in the 1-2keV band (Rate_band2_neg)ct/sstat.errordoublenullableCR3? The mean count-rate in the 2-10keV band (Rate_band3)ct/sphot.count;em.X-raydoublenullableE_CR3? The 1-sigma positive uncertainty on the mean count-rate in the 2-10keV band (Rate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_CR3[]? The 1-sigma negative uncertainty on the mean count-rate in the 2-10keV band (Rate_band3_neg)ct/sstat.errordoublenullableCt0? The total number of counts in the source region in the 0.3-10keV band (Counts_band0)ctphot.count;em.X-rayintnullableCt1? The total number of counts in the source region in the 0.3-1keV band (Counts_band1)ctphot.count;em.X-rayintnullableCt2? The total number of counts in the source region in the 1-2keV band (Counts_band2)ctphot.count;em.X-rayintnullableCt3? The total number of counts in the source region in the 2-10keV band (Counts_band3)ctphot.count;em.X-rayintnullablebgCt0? The total number of background counts expected in the source region in the 0.3-10keV band (BgCounts_band0)ctphot.count;em.X-raydoublenullablebgCt1? The total number of background counts expected in the source region in the 0.3-1keV band (BgCounts_band1)ctphot.count;em.X-raydoublenullablebgCt2? The total number of background counts expected in the source region in the 1-2keV band (BgCounts_band2)ctphot.count;em.X-raydoublenullablebgCt3? The total number of background counts expected in the source region in the 2-10keV band (BgCounts_band3)ctphot.count;em.X-raydoublenullableCF0? The PSF correction factor in the 0.3-10keV band (RateCF_band0)instr.paramfloatnullableCF1? The PSF correction factor in the 0.3-1keV band (RateCF_band1)instr.paramfloatnullableCF2? The PSF correction factor in the 1-2keV band (RateCF_band2)instr.paramfloatnullableCF3? The PSF correction factor in the 2-10keV band (RateCF_band3)instr.paramfloatnullableFUL0? The 3-sigma upper confidence limit on the count-rate in the 0.3-10keV band (UL_band0)ct/sphot.flux;em.X-raydoublenullableFUL1? The 3-sigma upper confidence limit on the count-rate in the 0.3-1keV band (UL_band1)ct/sphot.flux;em.X-raydoublenullableFUL2? The 3-sigma upper confidence limit on the count-rate in the 1-2keV band (UL_band2)ct/sphot.flux;em.X-raydoublenullableFUL3? The 3-sigma upper confidence limit on the count-rate in the 2-10keV band (UL_band3)ct/sphot.flux;em.X-raydoublenullablePCR0? The peak count-rate in the 0.3-10keV band (PeakRate_band0)ct/sphot.count;em.X-raydoublenullableE_PCR0? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-10keV band (PeakRate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_PCR0[]? The 1-sigma negative uncertainty on the peak count-rate in the 0.3-10keV band (PeakRate_band0_neg)ct/sstat.errordoublenullablePCR1? The peak count-rate in the 0.3-1keV band (PeakRate_band1)ct/sphot.count;em.X-raydoublenullableE_PCR1? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-1keV band (PeakRate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_PCR1[]? The 1-sigma negative uncertainty on the peak count-rate in the 0.3-1keV band (PeakRate_band1_neg)ct/sstat.errordoublenullablePCR2? The peak count-rate in the 1-2keV band (PeakRate_band2)ct/sphot.count;em.X-raydoublenullableE_PCR2? The 1-sigma positive uncertainty on the peak count-rate in the 1-2keV band (PeakRate_band2_pos)ct/sstat.error;stat.maxdoublenullablee_PCR2[]? The 1-sigma negative uncertainty on the peak count-rate in the 1-2keV band (PeakRate_band2_neg)ct/sstat.errordoublenullablePCR3? The peak count-rate in the 2-10keV band (PeakRate_band3)ct/sphot.count;em.X-raydoublenullableE_PCR3? The 1-sigma positive uncertainty on the peak count-rate in the 2-10keV band (PeakRate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_PCR3[]? The 1-sigma negative uncertainty on the peak count-rate in the 2-10keV band (PeakRate_band3_neg)ct/sstat.errordoublenullableNHgThe Galactic absorption column in the direction of the source, from Willingale et al (2013) (GalacticNH)cm**-2phys.absorption.galdoublePcstS0? The probability that the source count-rate in the 0.3-10keV band does not vary between snapshots (PvarPchiSnapshot_band0) (6)src.var.indexdoublenullablePcstS1? The probability that the source count-rate in the 0.3-1keV band does not vary between snapshots (PvarPchiSnapshot_band1) (6)src.var.indexdoublenullablePcstS2? The probability that the source count-rate in the 1-2keV band does not vary between snapshots (PvarPchiSnapshot_band2) (6)src.var.indexdoublenullablePcstS3? The probability that the source count-rate in the 2-10keV band does not vary between snapshots (PvarPchiSnapshot_band3) (6)src.var.indexdoublenullablePcstSHR1? The probability that the source HR1 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR1) (6)src.var.indexdoublenullablePcstSHR2? The probability that the source HR2 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR2) (6)src.var.indexdoublenullablePcst0? The probability that the source count-rate in the 0.3-10keV band does not vary between observations (PvarPchiObsID_band0) (6)src.var.indexdoublenullablePcst1? The probability that the source count-rate in the 0.3-1keV band does not vary between observations (PvarPchiObsID_band1) (6)src.var.indexdoublenullablePcst2? The probability that the source count-rate in the 1-2keV band does not vary between observations (PvarPchiObsID_band2) (6)src.var.indexdoublenullablePcst3? The probability that the source count-rate in the 2-10keV band does not vary between observations (PvarPchiObsID_band3) (6)src.var.indexdoublenullablePcstHR1? The probability that the source HR1 hardness ratio does not vary between observations (PvarPchiObsID_HR1) (6)src.var.indexdoublenullablePcstHR2? The probability that the source HR2 hardness ratio does not vary between observations (PvarPchiObsID_HR2) (6)src.var.indexdoublenullablePow? Which method of determining the spectral properties assuming a power-law was used (WhichPow) (7)meta.codeintnullableAPEC? Which method of determining the spectral properties assuming an APEC was used (WhichAPEC) (7)meta.codeintnullableCFO0? Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming a power-law spectrum (PowECFO)mJ.m**-2.count**-1instr.paramdoublenullableFPO0? The mean 0.3-10keV observed flux assuming a power-law spectrum (PowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPO0? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming a power-law spectrum (PowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPO0[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming a power-law spectrum (PowFlux_neg)mW.m**-2stat.errordoublenullableECFO0? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming an APEC spectrum (APECECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableFAO0? The mean 0.3-10keV observed flux assuming an APEC spectrum (APECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAO0? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming an APEC spectrum (APECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAO0[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming an APEC spectrum (APECFlux_neg)mW.m**-2stat.errordoublenullableFpPO0? The peak 0.3-10keV observed flux assuming a power-law spectrum (PowPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpPO0? The 1-sigma positive uncertainty on the peak 0.3-10keV observed flux assuming a power-law spectrum (PowPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpPO0[]? The 1-sigma negative uncertainty on the peak 0.3-10keV observed flux assuming a power-law spectrum (PowPeakFlux_neg)mW.m**-2stat.errordoublenullableFpAO0? The peak 0.3-10keV observed flux assuming an APEC spectrum (APECPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpAO0? The 1-sigma positive uncertainty on the peak 0.3-10keV observed flux assuming an APEC spectrum (APECPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpAO0[]? The 1-sigma negative uncertainty on the peak 0.3-10keV observed flux assuming an APEC spectrum (APECPeakFlux_neg)mW.m**-2stat.errordoublenullableCECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the canned power-law spectrum (FixedPowECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableCECFU? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the canned power-law spectrum (FixedPowECFU)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableFCOP0? The mean 0.3-10keV 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 0.3-10keV 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 0.3-10keV observed flux assuming the canned power-law spectrum (FixedPowFlux_neg)mW.m**-2stat.errordoublenullableFCUP0? The mean 0.3-10keV 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 0.3-10keV 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 0.3-10keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableAECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the canned APEC spectrum (FixedAPECECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableAECFU? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the canned APEC spectrum (FixedAPECECFU)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableFCAO1? The mean 0.3-10keV observed flux assuming the canned APEC spectrum (FixedAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCAO1? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCAO1[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_neg)mW.m**-2stat.errordoublenullablePECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFO)mJ.m**-2.count**-1arith.factordoublenullablePECFU? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFU)mJ.m**-2.count**-1arith.factordoublenullableNH1H? 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.errordoublenullableGam1? The spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma)spect.indexdoublenullableE_Gam1[]? 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_Gam1[]? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_neg)stat.errordoublenullableFIPO1? The mean 0.3-10keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPO1? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPO1[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_neg)mW.m**-2stat.errordoublenullableFIPU1? The mean 0.3-10keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPU1? The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPU1[]? The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableIPECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullablee_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.errordoublenullableFAIO1? The mean 0.3-10keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAIO1? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAIO1[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_neg)mW.m**-2stat.errordoublenullableP1? The probability that the HR values of this source could be obtained if the true spectrum is an absorbed power-law (P_pow)stat.probabilityfloatnullableP2? The probability that the HR values of this source could be obtained if the true spectrum is an APEC (P_APEC)stat.probabilityfloatnullableFPECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFO)mJ.m**-2.count**-1phot.flux;em.X-raydoublenullableGamma? 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) (8)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) (8)stat.errordoublenullableFPCO0? The mean 0.3-10keV 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 0.3-10keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_pos) (8)mW.m**-2stat.error;stat.maxdoublenullablee_FPCO0[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_neg) (8)mW.m**-2stat.errordoublenullableCstat? The C-statistic from the power-law spectral fit to the custom-built spectrum (FittedPowCstat)meta.codefloatnullablechi2r? 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 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullablekTAC? The temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT)keVspect.indexdoublenullableE_kTAC[]? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_pos) (8)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) (8)keVstat.errordoublenullableFACO0? The mean 0.3-10keV 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 0.3-10keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_pos) (8)mW.m**-2stat.error;stat.maxdoublenullablee_FACO0[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_neg) (8)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)stat.fit.dofintnullablechi2rA? The Churazov-weighted reduced chi^2^ from the APEC spectral fit to the custom-built spectrum (FittedAPECReducedChi2)stat.fit.chi2doublenullableHasSpec? Whether a custom-built spectrum was created for this source (HasSpec)meta.codeintnullableNext? The number of external sources found to agree spatially with this one at the 3-sigma level (NumExternalMatches)meta.numberintnullableNext2? The number of external sources found to agree spatially with this one at the 3-sigma level, excluding 2MASS, USNO-B1 and ALLWISE matches (NumExternalMatches_slim)meta.numberintnullableROSHRI? Whether the sources is spatially within 3 sigma of a source in the Rosat HRI catalogue (Cat. IX/28) (MatchInROSHRI)meta.noteintnullable2RXS? Whether the sources is spatially within 3 sigma of a source in the 2RXS catalogue (Cat. J/A+A/588/A103) (MatchIn2RXS)meta.noteintnullable3XMMDR8? Whether the sources is spatially within 3 sigma of a source in the 3XMM-DR8 catalogue (Cat. IX/55) (MatchIn3XMMDR8)meta.noteintnullable3XMMStack? Whether the sources is spatially within 3 sigma of a source in the 3XMM-DR7s (stacked) catalogue (Cat. IX/56) (MatchIn3XMM_Stack)meta.noteintnullableXMMSL2? Whether the sources is spatially within 3 sigma of a source in the XMMSL2 catalogue (Cat. IX/53) (MatchInXMMSL2)meta.noteintnullableSwiftFT? Whether the sources is spatially within 3 sigma of a source in the SwiftFT catalogue (Cat. J/A+A/528/A122) (MatchInSwiftFT)meta.noteintnullable1SWXRT? Whether the sources is spatially within 3 sigma of a source in the 1SWXRT catalogue (Cat. J/A+A/551/A142) (MatchIn1SWXRT)meta.noteintnullableXRTGRB? Whether the sources is spatially within 3 sigma of an XRT GRB afterglow (MatchInXRTGRB)meta.noteintnullableSDSSQSO? Whether the sources is spatially within 3 sigma of a source in the SDSS QSO DR14 catalogue (MatchInSDSSQSO)meta.noteintnullable2MASS? Whether the sources is spatially within 3 sigma of a source in the 2MASS catalogue (Cat. II/246) (MatchIn2MASS)meta.noteintnullableUSNOB1? Whether the sources is spatially within 3 sigma of a source in the USNO-B1 catalogue (Cat. I/284) (MatchInUSNOB1)meta.noteintnullable2CSC? Whether the sources is spatially within 3 sigma of a source in the 2CSC catalogue (MatchIn2CSC)meta.noteintnullable1SXPS? Whether the sources is spatially within 3 sigma of a source in the 1SXPS catalogue (Cat. IX/43) (MatchIn1SXPS)meta.noteintnullableALLWISE? Whether the sources is spatially within 3 sigma of a source in the ALLWISE catalogue (Cat. II/328) (MatchInALLWISE)meta.noteintnullableONamesThe list of other sources which may be aliases of this one (PotentialAliasList)meta.idcharCFU0Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming a power-law spectrum (PowECFU)mJ.m**-2.count**-1instr.paramcharFPU0The mean 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux)mW.m**-2phot.flux;em.X-raychare_FPU0The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_neg)mW.m**-2stat.errorcharECFU0The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming an APEC spectrum (APECECFU)mJ.m**-2.count**-1arith.factor;phys.energycharFAU0The mean 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FAU0The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FAU0The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_neg)mW.m**-2stat.errorcharFpPU0The peak 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FpPU0The 1-sigma positive uncertainty on the peak 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FpPU0The 1-sigma negative uncertainty on the peak 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_neg)mW.m**-2stat.errorcharFpAU0The peak 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FpAU0The 1-sigma positive uncertainty on the peak 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FpAU0The 1-sigma negative uncertainty on the peak 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_neg)mW.m**-2stat.errorcharFCAU1The mean 0.3-10keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FCAU1The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FCAU1The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_neg)mW.m**-2stat.errorcharIPECFUThe Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFU)mJ.m**-2.count**-1arith.factor;phys.energycharNH2AThe hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH)cm**-2phys.columnDensitycharE_NH2AThe 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_pos)cm**-2stat.error;stat.maxcharFAIU1The mean 0.3-10keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FAIU1The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FAIU1The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_neg)mW.m**-2stat.errorcharFPECFUThe Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFU)mJ.m**-2.count**-1phot.flux;em.X-raycharNH2CThe hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH)cm**-2phys.columnDensitycharE_NH2CThe 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_pos) (8)cm**-2stat.error;stat.maxchare_NH2CThe 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_neg) (8)cm**-2stat.errorcharFPCU0The mean 0.3-10keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FPCU0The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_pos) (8)mW.m**-2stat.error;stat.maxchare_FPCU0The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_neg) (8)mW.m**-2stat.errorcharACECFUThe Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFU)mJ.m**-2.count**-1arith.factor;phys.energycharNH2ACThe hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH)cm**-2phys.columnDensitycharE_NH2ACThe 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_pos) (8)cm**-2stat.error;stat.maxchare_NH2ACThe 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_neg) (8)cm**-2stat.errorcharFACU0The mean 0.3-10keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FACU0The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_pos) (8)mW.m**-2stat.error;stat.maxchare_FACU0The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_neg) (8)mW.m**-2stat.errorchar
IX/58/2sxpscleThe 2SXPS Catalogue of Swift X-ray telescope Point Sources "clean" versionGLONGalactic longitude (l)degpos.galactic.lonPcstS2? The probability that the source count-rate in the 1-2keV band does not vary between snapshots (PvarPchiSnapshot_band2) (6)src.var.indexdoublenullableFIPU1? The mean 0.3-10keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux)mW.m**-2phot.flux;em.X-raydoublenullableXRTGRB? Whether the sources is spatially within 3 sigma of an XRT GRB afterglow (MatchInXRTGRB)meta.noteintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint2SXPSNumerical unique source identifier within 2SXPS (2SXPS_ID)meta.id;meta.mainintRAJ2000Right 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.errorfloatA[0/1] Provenance of source astrometry. 0=Swift star tracker, 1=XRT/2MASS astrometry (AstromType)meta.ref;pos.frameintGLATGalactic latitude (b)degpos.galactic.latdoubleOffAxisThe mean angular distance of the source from the XRT boresight in all observations within which the source was detected (MeanOffAxisAngle) (1)arcminpos.angDistance;stat.meanfloatDNNThe distance to the closest 2SXPS source to this one (NearestNeighbour)arcsecpos.angDistancedoubleDNNOKThe distance to the closest 2SXPS source to this one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour)arcsecpos.angDistancedoublet.expThe total exposure at the source location in the catalogue (Exposure)stime.expointt.start1The UTC date & time of the start of the first observation in 2SXPS which covered the source location (FirstObsDate)stime.epochnullablet.stop1The UTC date & time of the end of the last observation in 2SXPS which covered the source location (LastObsDate)stime.epochnullabletime.start1The time of the start of the first observation in 2SXPS which covered the source location, in Swift Mission Elapsed Time (FirstObsMET) (2)stime.expolongtime.stop1The time of the end of the last observation in 2SXPS which covered the source location in, Swift Mission Elapsed Time (LastObsMET) (2)stime.expolongt.start2The UTC date & time of the start of the first observation in 2SXPS in which the source count rate is inconsistent with 0 at the 3-sigma level (FirstDetDate)stime.epochnullablet.stop2The UTC date & time of the end of the last observation in 2SXPS in which the source count rate is inconsistent with 0 at the 3-sigma level (LastDetDate)stime.epochnullabletime.start2The time of the start of the first observation in 2SXPS in which the source count rate is inconsistent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (FirstDetMET)(2)stime.expolongtime.stop2The time of the end of the last observation in 2SXPS in which the source count rate is inconsistent with 0 at the 3-sigma level, in Swift Mission Elapsed Time (LastDetMET) (2)stime.expolongt.start3The UTC date & time of the start of the first observation in 2SXPS 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 2SXPS in which the source is detected in the blind search (LastBlindDetDate)stime.epochnullabletime.start3The time of the start of the first observation in 2SXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (FirstBlindDetMET) (2)stime.expolongtime.stop3The time of the end of the last observation in 2SXPS in which the source is detected in the blind search, in Swift Mission Elapsed Time (LastBlindDetMET) (2)stime.expolongNObsThe number of observations covering this source's position (NumObs)meta.numberintNBlindThe number of observations in which this source was found in a blind search (NumBlindDetObs)meta.numberintNDetThe number of observations in which this source is detected (NumDetObs)meta.numberintNBestThe ID of the 'best' detection (BestDetectionID)meta.numberintF0Whether the count-rate in the 0.3-10keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band0)meta.codeintF1Whether the count-rate in the 0.3-1keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band1)meta.codeintF2Whether the count-rate in the 1-2keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band2)meta.codeintF3Whether the count-rate in the 2-10keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band3)meta.codeintDet? The final source detection flag (DetFlag) (3)meta.code.error;phys.atmol.finalintnullableFField? The final fieldFlag for this source (FieldFlag) (4)meta.codeintnullableDet0? The final detection flag the 0.3-10keV band (DetFlag_band0) (3)meta.code.qualintnullableDet1? The final detection flag the 0.3-1keV band (DetFlag_band1) (3)meta.code.qualintnullableDet2? The final detection flag in the 1-2keV band (DetFlag_band2) (3)meta.code.qualintnullableDet3? The final detection flag in the 2-10keV band (DetFlag_band3) (3)meta.code.qualintnullableWarningThe worst optical loading warning from all detections of this source (5)magmeta.codedoubleDetSLWWhether 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.codeintCR0? The mean count-rate in the 0.3-10keV band (Rate_band0)ct/sphot.count;em.X-raydoublenullableE_CR0? The 1-sigma positive uncertainty on the mean count-rate in the 0.3-10keV band (Rate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_CR0[]? The 1-sigma negative uncertainty on the mean count-rate in the 0.3-10keV 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.maxfloatnullablee_HR1[]? The 1-sigma negative uncertainty on the aggregate HR1 hardness ratio of the source (HR1_neg)stat.errorfloatnullableHR2? 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.maxfloatnullablee_HR2[]? The 1-sigma negative uncertainty on the aggregate HR2 hardness ratio of the source (HR2_neg)stat.errorfloatnullableCR1? The mean count-rate in the 0.3-1keV band (Rate_band1)ct/sphot.count;em.X-raydoublenullableE_CR1? The 1-sigma positive uncertainty on the mean count-rate in the 0.3-1keV band (Rate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_CR1[]? The 1-sigma negative uncertainty on the mean count-rate in the 0.3-1keV band (Rate_band1_neg)ct/sstat.errordoublenullableCR2? The mean count-rate in the 1-2keV band (Rate_band2)ct/sphot.count;em.X-raydoublenullableE_CR2? The 1-sigma positive uncertainty on the mean count-rate in the 1-2keV band (Rate_band2_pos)ct/sstat.error;stat.maxdoublenullablee_CR2[]? The 1-sigma negative uncertainty on the mean count-rate in the 1-2keV band (Rate_band2_neg)ct/sstat.errordoublenullableCR3? The mean count-rate in the 2-10keV band (Rate_band3)ct/sphot.count;em.X-raydoublenullableE_CR3? The 1-sigma positive uncertainty on the mean count-rate in the 2-10keV band (Rate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_CR3[]? The 1-sigma negative uncertainty on the mean count-rate in the 2-10keV band (Rate_band3_neg)ct/sstat.errordoublenullableCt0? The total number of counts in the source region in the 0.3-10keV band (Counts_band0)ctphot.count;em.X-rayintnullableCt1? The total number of counts in the source region in the 0.3-1keV band (Counts_band1)ctphot.count;em.X-rayintnullableCt2? The total number of counts in the source region in the 1-2keV band (Counts_band2)ctphot.count;em.X-rayintnullableCt3? The total number of counts in the source region in the 2-10keV band (Counts_band3)ctphot.count;em.X-rayintnullablebgCt0? The total number of background counts expected in the source region in the 0.3-10keV band (BgCounts_band0)ctphot.count;em.X-raydoublenullablebgCt1? The total number of background counts expected in the source region in the 0.3-1keV band (BgCounts_band1)ctphot.count;em.X-raydoublenullablebgCt2? The total number of background counts expected in the source region in the 1-2keV band (BgCounts_band2)ctphot.count;em.X-raydoublenullablebgCt3? The total number of background counts expected in the source region in the 2-10keV band (BgCounts_band3)ctphot.count;em.X-raydoublenullableCF0? The PSF correction factor in the 0.3-10keV band (RateCF_band0)instr.paramfloatnullableCF1? The PSF correction factor in the 0.3-1keV band (RateCF_band1)instr.paramfloatnullableCF2? The PSF correction factor in the 1-2keV band (RateCF_band2)instr.paramfloatnullableCF3? The PSF correction factor in the 2-10keV band (RateCF_band3)instr.paramfloatnullableFUL0? The 3-sigma upper confidence limit on the count-rate in the 0.3-10keV band (UL_band0)ct/sphot.flux;em.X-raydoublenullableFUL1? The 3-sigma upper confidence limit on the count-rate in the 0.3-1keV band (UL_band1)ct/sphot.flux;em.X-raydoublenullableFUL2? The 3-sigma upper confidence limit on the count-rate in the 1-2keV band (UL_band2)ct/sphot.flux;em.X-raydoublenullableFUL3? The 3-sigma upper confidence limit on the count-rate in the 2-10keV band (UL_band3)ct/sphot.flux;em.X-raydoublenullablePCR0? The peak count-rate in the 0.3-10keV band (PeakRate_band0)ct/sphot.count;em.X-raydoublenullableE_PCR0? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-10keV band (PeakRate_band0_pos)ct/sstat.error;stat.maxdoublenullablee_PCR0[]? The 1-sigma negative uncertainty on the peak count-rate in the 0.3-10keV band (PeakRate_band0_neg)ct/sstat.errordoublenullablePCR1? The peak count-rate in the 0.3-1keV band (PeakRate_band1)ct/sphot.count;em.X-raydoublenullableE_PCR1? The 1-sigma positive uncertainty on the peak count-rate in the 0.3-1keV band (PeakRate_band1_pos)ct/sstat.error;stat.maxdoublenullablee_PCR1[]? The 1-sigma negative uncertainty on the peak count-rate in the 0.3-1keV band (PeakRate_band1_neg)ct/sstat.errordoublenullablePCR2? The peak count-rate in the 1-2keV band (PeakRate_band2)ct/sphot.count;em.X-raydoublenullableE_PCR2? The 1-sigma positive uncertainty on the peak count-rate in the 1-2keV band (PeakRate_band2_pos)ct/sstat.error;stat.maxdoublenullablee_PCR2[]? The 1-sigma negative uncertainty on the peak count-rate in the 1-2keV band (PeakRate_band2_neg)ct/sstat.errordoublenullablePCR3? The peak count-rate in the 2-10keV band (PeakRate_band3)ct/sphot.count;em.X-raydoublenullableE_PCR3? The 1-sigma positive uncertainty on the peak count-rate in the 2-10keV band (PeakRate_band3_pos)ct/sstat.error;stat.maxdoublenullablee_PCR3[]? The 1-sigma negative uncertainty on the peak count-rate in the 2-10keV band (PeakRate_band3_neg)ct/sstat.errordoublenullableNHgThe Galactic absorption column in the direction of the source, from Willingale et al (2013) (GalacticNH)cm**-2phys.absorption.galdoublePcstS0? The probability that the source count-rate in the 0.3-10keV band does not vary between snapshots (PvarPchiSnapshot_band0) (6)src.var.indexdoublenullablePcstS1? The probability that the source count-rate in the 0.3-1keV band does not vary between snapshots (PvarPchiSnapshot_band1) (6)src.var.indexdoublenullablePcstS3? The probability that the source count-rate in the 2-10keV band does not vary between snapshots (PvarPchiSnapshot_band3) (6)src.var.indexdoublenullablePcstSHR1? The probability that the source HR1 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR1) (6)src.var.indexdoublenullablePcstSHR2? The probability that the source HR2 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR2) (6)src.var.indexdoublenullablePcst0? The probability that the source count-rate in the 0.3-10keV band does not vary between observations (PvarPchiObsID_band0) (6)src.var.indexdoublenullablePcst1? The probability that the source count-rate in the 0.3-1keV band does not vary between observations (PvarPchiObsID_band1) (6)src.var.indexdoublenullablePcst2? The probability that the source count-rate in the 1-2keV band does not vary between observations (PvarPchiObsID_band2) (6)src.var.indexdoublenullablePcst3? The probability that the source count-rate in the 2-10keV band does not vary between observations (PvarPchiObsID_band3) (6)src.var.indexdoublenullablePcstHR1? The probability that the source HR1 hardness ratio does not vary between observations (PvarPchiObsID_HR1) (6)src.var.indexdoublenullablePcstHR2? The probability that the source HR2 hardness ratio does not vary between observations (PvarPchiObsID_HR2) (6)src.var.indexdoublenullablePow? Which method of determining the spectral properties assuming a power-law was used (WhichPow) (7)meta.codeintnullableAPEC? Which method of determining the spectral properties assuming an APEC was used (WhichAPEC) (7)meta.codeintnullableCFO0? Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming a power-law spectrum (PowECFO)mJ.m**-2.count**-1instr.paramdoublenullableFPO0? The mean 0.3-10keV observed flux assuming a power-law spectrum (PowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FPO0? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming a power-law spectrum (PowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FPO0[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming a power-law spectrum (PowFlux_neg)mW.m**-2stat.errordoublenullableECFO0? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming an APEC spectrum (APECECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableFAO0? The mean 0.3-10keV observed flux assuming an APEC spectrum (APECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAO0? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming an APEC spectrum (APECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAO0[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming an APEC spectrum (APECFlux_neg)mW.m**-2stat.errordoublenullableFAU0The mean 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux)mW.m**-2phot.flux;em.X-raycharFpPO0? The peak 0.3-10keV observed flux assuming a power-law spectrum (PowPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpPO0? The 1-sigma positive uncertainty on the peak 0.3-10keV observed flux assuming a power-law spectrum (PowPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpPO0[]? The 1-sigma negative uncertainty on the peak 0.3-10keV observed flux assuming a power-law spectrum (PowPeakFlux_neg)mW.m**-2stat.errordoublenullableFpAO0? The peak 0.3-10keV observed flux assuming an APEC spectrum (APECPeakFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FpAO0? The 1-sigma positive uncertainty on the peak 0.3-10keV observed flux assuming an APEC spectrum (APECPeakFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FpAO0[]? The 1-sigma negative uncertainty on the peak 0.3-10keV observed flux assuming an APEC spectrum (APECPeakFlux_neg)mW.m**-2stat.errordoublenullableCECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the canned power-law spectrum (FixedPowECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableCECFU? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the canned power-law spectrum (FixedPowECFU)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableFCOP0? The mean 0.3-10keV 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 0.3-10keV 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 0.3-10keV observed flux assuming the canned power-law spectrum (FixedPowFlux_neg)mW.m**-2stat.errordoublenullableFCUP0? The mean 0.3-10keV 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 0.3-10keV 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 0.3-10keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableAECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the canned APEC spectrum (FixedAPECECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableAECFU? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the canned APEC spectrum (FixedAPECECFU)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableFCAO1? The mean 0.3-10keV observed flux assuming the canned APEC spectrum (FixedAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FCAO1? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FCAO1[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_neg)mW.m**-2stat.errordoublenullablePECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFO)mJ.m**-2.count**-1arith.factordoublenullablePECFU? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the power-law spectrum interpolated from the HRs (InterpPowECFU)mJ.m**-2.count**-1arith.factordoublenullableNH1H? 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.errordoublenullableGam1? The spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma)spect.indexdoublenullableE_Gam1[]? 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_Gam1[]? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_neg)stat.errordoublenullableFIPO1? The mean 0.3-10keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FIPO1? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPO1[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux_neg)mW.m**-2stat.errordoublenullableE_FIPU1? The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FIPU1[]? The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux_neg)mW.m**-2stat.errordoublenullableIPECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullablee_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)keVspect.indexdoublenullableE_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.errordoublenullableFAIO1? The mean 0.3-10keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux)mW.m**-2phot.flux;em.X-raydoublenullableE_FAIO1? The 1-sigma positive uncertainty on the mean 0.3-10keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_pos)mW.m**-2stat.error;stat.maxdoublenullablee_FAIO1[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_neg)mW.m**-2stat.errordoublenullableP1? The probability that the HR values of this source could be obtained if the true spectrum is an absorbed power-law (P_pow)stat.probabilityfloatnullableP2? The probability that the HR values of this source could be obtained if the true spectrum is an APEC (P_APEC)stat.probabilityfloatnullableFPECFO? The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFO)mJ.m**-2.count**-1phot.flux;em.X-raydoublenullableGamma? 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) (8)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) (8)stat.errordoublenullableFPCO0? The mean 0.3-10keV 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 0.3-10keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_pos) (8)mW.m**-2stat.error;stat.maxdoublenullablee_FPCO0[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux_neg) (8)mW.m**-2stat.errordoublenullableCstat? The C-statistic from the power-law spectral fit to the custom-built spectrum (FittedPowCstat)meta.codefloatnullableDOF? The number of degrees of freedom in the power-law spectral fit to the custom-built spectrum (FittedPowDOF)stat.fit.dofintnullablechi2r? 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 0.3-10keV count-rate to 0.3-10keV observed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFO)mJ.m**-2.count**-1arith.factor;phys.energydoublenullableNH2ACThe hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH)cm**-2phys.columnDensitycharkTAC? The temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT)keVspect.indexdoublenullableE_kTAC[]? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_pos) (8)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) (8)keVstat.errordoublenullableFACO0? The mean 0.3-10keV 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 0.3-10keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_pos) (8)mW.m**-2stat.error;stat.maxdoublenullablee_FACO0[]? The 1-sigma negative uncertainty on the mean 0.3-10keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux_neg) (8)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)stat.fit.dofintnullablechi2rA? The Churazov-weighted reduced chi^2^ from the APEC spectral fit to the custom-built spectrum (FittedAPECReducedChi2)stat.fit.chi2doublenullableHasSpec? Whether a custom-built spectrum was created for this source (HasSpec)meta.codeintnullableNext? The number of external sources found to agree spatially with this one at the 3-sigma level (NumExternalMatches)meta.numberintnullableNext2? The number of external sources found to agree spatially with this one at the 3-sigma level, excluding 2MASS, USNO-B1 and ALLWISE matches (NumExternalMatches_slim)meta.numberintnullableROSHRI? Whether the sources is spatially within 3 sigma of a source in the Rosat HRI catalogue (Cat. IX/28) (MatchInROSHRI)meta.noteintnullable2RXS? Whether the sources is spatially within 3 sigma of a source in the 2RXS catalogue (Cat. J/A+A/588/A103) (MatchIn2RXS)meta.noteintnullable3XMMDR8? Whether the sources is spatially within 3 sigma of a source in the 3XMM-DR8 catalogue (Cat. IX/55) (MatchIn3XMMDR8)meta.noteintnullable3XMMStack? Whether the sources is spatially within 3 sigma of a source in the 3XMM-DR7s (stacked) catalogue (Cat. IX/56) (MatchIn3XMM_Stack)meta.noteintnullableXMMSL2? Whether the sources is spatially within 3 sigma of a source in the XMMSL2 catalogue (Cat. IX/53) (MatchInXMMSL2)meta.noteintnullableSwiftFT? Whether the sources is spatially within 3 sigma of a source in the SwiftFT catalogue (Cat. J/A+A/528/A122) (MatchInSwiftFT)meta.noteintnullable1SWXRT? Whether the sources is spatially within 3 sigma of a source in the 1SWXRT catalogue (Cat. J/A+A/551/A142) (MatchIn1SWXRT)meta.noteintnullableSDSSQSO? Whether the sources is spatially within 3 sigma of a source in the SDSS QSO DR14 catalogue (MatchInSDSSQSO)meta.noteintnullable2MASS? Whether the sources is spatially within 3 sigma of a source in the 2MASS catalogue (Cat. II/246) (MatchIn2MASS)meta.noteintnullableUSNOB1? Whether the sources is spatially within 3 sigma of a source in the USNO-B1 catalogue (Cat. I/284) (MatchInUSNOB1)meta.noteintnullable2CSC? Whether the sources is spatially within 3 sigma of a source in the 2CSC catalogue (MatchIn2CSC)meta.noteintnullable1SXPS? Whether the sources is spatially within 3 sigma of a source in the 1SXPS catalogue (Cat. IX/43) (MatchIn1SXPS)meta.noteintnullableALLWISE? Whether the sources is spatially within 3 sigma of a source in the ALLWISE catalogue (Cat. II/328) (MatchInALLWISE)meta.noteintnullableIAUNameIAU-format name, 2SXPS JHHMMSS+-ddmmsss (IAUName)meta.idcharONamesThe list of other sources which may be aliases of this one (PotentialAliasList)meta.idcharCFU0Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming a power-law spectrum (PowECFU)mJ.m**-2.count**-1instr.paramcharFPU0The mean 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FPU0The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FPU0The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_neg)mW.m**-2stat.errorcharECFU0The Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming an APEC spectrum (APECECFU)mJ.m**-2.count**-1arith.factor;phys.energycharE_FAU0The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FAU0The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_neg)mW.m**-2stat.errorcharFpPU0The peak 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FpPU0The 1-sigma positive uncertainty on the peak 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FpPU0The 1-sigma negative uncertainty on the peak 0.3-10keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_neg)mW.m**-2stat.errorcharFpAU0The peak 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FpAU0The 1-sigma positive uncertainty on the peak 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FpAU0The 1-sigma negative uncertainty on the peak 0.3-10keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_neg)mW.m**-2stat.errorcharFCAU1The mean 0.3-10keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FCAU1The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FCAU1The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_neg)mW.m**-2stat.errorcharIPECFUThe Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the APEC spectrum interpolated from the HRs (InterpAPECECFU)mJ.m**-2.count**-1arith.factor;phys.energycharNH2AThe hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH)cm**-2phys.columnDensitycharE_NH2AThe 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_pos)cm**-2stat.error;stat.maxcharFAIU1The mean 0.3-10keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FAIU1The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_pos)mW.m**-2stat.error;stat.maxchare_FAIU1The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_neg)mW.m**-2stat.errorcharFPECFUThe Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowECFU)mJ.m**-2.count**-1phot.flux;em.X-raycharNH2CThe hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH)cm**-2phys.columnDensitycharE_NH2CThe 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_pos) (8)cm**-2stat.error;stat.maxchare_NH2CThe 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH_neg) (8)cm**-2stat.errorcharFPCU0The mean 0.3-10keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FPCU0The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_pos) (8)mW.m**-2stat.error;stat.maxchare_FPCU0The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux_neg) (8)mW.m**-2stat.errorcharACECFUThe Energy Conversion Factor from 0.3-10keV count-rate to 0.3-10keV unabsorbed flux, assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECECFU)mJ.m**-2.count**-1arith.factor;phys.energycharE_NH2ACThe 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_pos) (8)cm**-2stat.error;stat.maxchare_NH2ACThe 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_neg) (8)cm**-2stat.errorcharFACU0The mean 0.3-10keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux)mW.m**-2phot.flux;em.X-raycharE_FACU0The 1-sigma positive uncertainty on the mean 0.3-10keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_pos) (8)mW.m**-2stat.error;stat.maxchare_FACU0The 1-sigma negative uncertainty on the mean 0.3-10keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux_neg) (8)mW.m**-2stat.errorchar