VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

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J/MNRAS/518/174
  LSXPS Swift-XRT point sources and transients (Evans+, 2023)
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2023MNRAS.518..174E
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Post annotation 		img(gal)
1.J/MNRAS/518/174/sources(c)Sources table is the main LSXPS table (348599 rows)
2.J/MNRAS/518/174/sclean(c)Clean subset of the source table those with a best Det Flag of 0 or 1 for Good or Reasonable (229778 rows)
3.J/MNRAS/518/174/suclean(c)Ultraclean subset of the sclean table those with Det=0 and FField=0 (202939 rows)
4.J/MNRAS/518/174/datasets(c)Information about every individual datasets, observations and stacked images in LSXPS (284508 rows)
5.J/MNRAS/518/174/dclean(c)Subset of datasets.dat where FFlag=0 or 1 (270187 rows)
6.J/MNRAS/518/174/duclean(c)Subset of dclean where FFlag=0 (267428 rows)
7.J/MNRAS/518/174/detect(c)*Specific individual X-ray detections catalog in all band before combination to create sources (Note) (2792443 rows)
8.J/MNRAS/518/174/obsource*Details of the detections in an individual dataset, merged over all bands (Note) (1455404 rows)
9.J/MNRAS/518/174/xcorr(c)Details of the cross correlation between the LSXPS sources and other catalogues (1133795 rows)
10.J/MNRAS/518/174/oldstackDetails of the stacked images which have been superseded by newer data (25645 rows)
11.J/MNRAS/518/174/trans(c)Transient counterpart checked by the XRT team and classed into 'possible transient' categories (1238 rows)

Simple ConstraintList Of Constraints
 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1+2+3+7+8+9+11)LSXPS  Numerical unique source identifier within LSXPS (LSXPS_ID) (meta.id;meta.main)
  (1+2+3+11)IAUName (char) IAU-format name, LSXPS JHHMMSS s±ddmmsss (IAUName) (meta.id)
  (1+2+3+4+5+6+7+11)RAJ2000 deg (i) Right ascension (J2000) (RA) (pos.eq.ra;meta.main)
  (1+2+3+4+5+6+7+11)DEJ2000 deg (i) Declination (J2000) (Decl) (pos.eq.dec;meta.main)
  (1+2+3+7+11)Err90 arcsec Position uncertainty, 90% confidence, radial, assumed to be Rayleigh-distributed (Err90) (stat.error)
  (1+2+3)A  Provenance of the astrometry used to derive the source position (AstromType) (Note 1)   (meta.code)
  (1+2+3+4+5+6+7+11)GLON deg Galactic longitude (l) (pos.galactic.lon)
  (1+2+3+4+5+6+7+11)GLAT deg Galactic latitude (b) (pos.galactic.lat)
  (1+2+3+7)OffAxis arcmin (n) The mean angular distance of the source from the XRT boresight in all observations within which the source was detected (MeanOffAxisAngle) (pos.angDistance;stat.mean)
  (1+2+3+7+8)DNN arcsec The distance to the closest LSXPS source to this one (NearestNeighbour) (pos.angDistance)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3+7+8)DNNOK arcsec The distance to the closest LSXPS source to this one which is ranked Good or Reasonable and has no other DetFlag bits set (NearestOKNeighbour) (pos.angDistance)
  (1+2+3)NLSXPS  (n) The LSXPS_ID of the closest LSXPS source to this one (NearestNeighbour_ID) (meta.id.cross)
  (1+2+3)GoodNLSXPS  (n) 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.cross)
  (1+2+3)HPPIX  The Healpix pixel containing the source (NSIDE=128, ordering=RING) (HPPIX) (meta.id;instr)
  (1+2+3)t.exp s (n) The total exposure at the source location in the catalogue (Exposure) (time.expo)
  (1+2+3+4+5+6)t.start1 s (n)The UTC date & time of the start of the first observation in LSXPS which covered the source location (FirstObsDate) (time.epoch)
  (1+2+3+4+5+6)t.stop1 s (n)The UTC date & time of the end of the last observation in LSXPS which covered the source location (LastObsDate) (time.end;obs)
  (1+2+3+4+5+6)time.start1 s (n) The time of the start of the first observation in LSXPS which covered the source location, in Swift Mission Elapsed Time (FirstObsMET) (time.epoch)
  (1+2+3+4+5+6)time.stop1 s (n) The time of the end of the last observation in LSXPS which covered the source location in, Swift Mission Elapsed Time (LastObsMET) (time.epoch)
  (1+2+3)t.start2 s (n)The 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) (time.epoch)
  (1+2+3)t.stop2 s (n)The 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) (time.epoch)
  (1+2+3)time.start2 s (n) 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) (time.epoch)
  (1+2+3)time.stop2 s (n) 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) (time.epoch)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)t.start3 s (n)The UTC date & time of the start of the first observation in LSXPS in which the source is detected in the blind search (FirstBlindDetDate) (time.epoch)
  (1+2+3)t.stop3 s (n)The UTC date & time of the end of the last observation in LSXPS in which the source is detected in the blind search (LastBlindDetDate) (time.end;obs)
  (1+2+3)time.start3 s (n) 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) (time.epoch)
  (1+2+3)time.stop3 s (n) 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) (time.epoch)
  (1+2+3)NObs  (n) The number of observations covering the position of this source (NumObs) (meta.number)
  (1+2+3)NBlind  (n) The number of observations in which this source was found in a blind search (NumBlindDetObs) (meta.number)
  (1+2+3)NDet  (n) The number of observations in which this source is detected (NumDetObs) (meta.number)
  (1+2+3)IDBest  The ID of the 'best' detection, (cf the detection table) (BestDetectionID) (meta.id.cross)
  (1+2+3)F0  (n) Whether the count-rate in the 0.3-10 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band0) (meta.code)
  (1+2+3)F1  (n) Whether the count-rate in 0.3-1 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band1) (meta.code)
  (1+2+3)F2  (n) Whether the count-rate in 1-2 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band2) (meta.code)
  (1+2+3)F3  (n) Whether the count-rate in 2-10 keV band is inconsistent with 0 at the 3-sigma level (NonBlindDet_band3) (meta.code)
  (1+2+3)Det  The best detection flag from all detections of the source (DetFlag) (Note 2)   (meta.code)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)FField  The best field flag from all detections of the source (FieldFlag) (Note 3)   (meta.code)
  (1+2+3)Det0  The final detection flag 0.3-10 keV band (DetFlag_band0) (meta.code)
  (1+2+3)Det1  The final detection flag 0.3-1 keV band (DetFlag_band1) (meta.code)
  (1+2+3)Det2  The final detection flag in 1-2 keV band (DetFlag_band2) (meta.code)
  (1+2+3)Det3  The final detection flag in 2-10 keV band (DetFlag_band3) (meta.code)
  (1+2+3+7)Warning mag The worst optical loading warning from all detections of this source (OpticalLoadingWarning) (Note 4)   (phot.mag;em.opt)
  (1+2+3+7)DetSLW  Whether any detection of this source occurred within fitted stray light rings (StrayLightWarning) (meta.code)
  (1+2+3+7)DetNBSW  Whether any detection of this source occurred within the PSF wings of a bright object (NearBrightSourceWarning) (meta.code)
  (1+2+3)Dup  Whether this source is potentially an alias (i e duplicate) of another source (IsPotentialAlias) (meta.code)
  (1+2+3)AdDate s (n)(i) The date at which this source was added to LSXPS (WhenAdded) (time.epoch)
  (1+2+3)SDet  Whether the source was detected in the most recent observation of its location (StillDetected) (Note 5)   (meta.code)
  (1+2+3)Status  A bit-wise flag describing the processing status of the source data (ProcessedStatus) (meta.code)
  (1+2+3)ModDate s (n)The date at which this source was last analysed (WhenModified) (time.epoch)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)CR0 ct/s (n) The mean count-rate in 0.3-10 keV band (Rate_band0) (phot.count;arith.rate;em.X-ray)
  (1+2+3)E_CR0 ct/s (n) The 1-sigma positive uncertainty on the mean count-rate in the 0.3-10 keV band (Rateband0pos) (stat.error;stat.max)
  (1+2+3)e_CR0 ct/s (n) []? The 1-sigma negative uncertainty on the mean count-rate in 0.3-10 keV band (Rateband0neg) (stat.error)
  (1+2+3+8)HR1  (n) The aggregate HR1 hardness ratio of the source (HR1) (phot.flux;arith.ratio)
  (1+2+3+8)E_HR1  (n) []? The 1-sigma positive uncertainty on the aggregate HR1 hardness ratio of the source (HR1_pos) (stat.error;stat.max)
  (1+2+3+8)e_HR1  (n) []? The 1-sigma negative uncertainty on the aggregate HR1 hardness ratio of the source (HR1_neg) (stat.error)
  (1+2+3+8)HR2  (n) The aggregate HR2 hardness ratio of the source (HR2) (phot.flux;arith.ratio)
  (1+2+3+8)E_HR2  (n) []? The 1-sigma positive uncertainty on the aggregate HR2 hardness ratio of the source (HR2_pos) (stat.error;stat.max)
  (1+2+3+8)e_HR2  (n) []? The 1-sigma negative uncertainty on the aggregate HR2 hardness ratio of the source (HR2_neg) (stat.error)
  (1+2+3)CR1 ct/s (n) The mean count-rate in 0.3-1 keV band (Rate_band1) (phot.count;arith.rate;em.X-ray.soft)
  (1+2+3)E_CR1 ct/s (n) The 1-sigma positive uncertainty on the mean count-rate in 0.3-1 keV band (Rateband1pos) (stat.error;stat.max)
  (1+2+3)e_CR1 ct/s (n) []? The 1-sigma negative uncertainty on the mean count-rate in 0.3-1 keV band (Rateband1neg) (stat.error)
  (1+2+3)CR2 ct/s (n) The mean count-rate in the 1-2 keV band (Rate_band2) (phot.count;arith.rate;em.X-ray.soft)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)E_CR2 ct/s (n) The 1-sigma positive uncertainty on the mean count-rate in the 1-2 keV band (Rateband2pos) (stat.error;stat.max)
  (1+2+3)e_CR2 ct/s (n) []? The 1-sigma negative uncertainty on the mean count-rate in the 1-2 keV band (Rateband2neg) (stat.error)
  (1+2+3)CR3 ct/s (n) The mean count-rate in the 2-10 keV band (Rate_band3) (phot.count;arith.rate;em.X-ray.medium)
  (1+2+3)E_CR3 ct/s (n) The 1-sigma positive uncertainty on the mean count-rate in the 2-10 keV band (Rateband3pos) (stat.error;stat.max)
  (1+2+3)e_CR3 ct/s (n) []? The 1-sigma negative uncertainty on the mean count-rate in 2-10 keV band (Rateband3neg) (stat.error)
  (1+2+3)Ct0 ct (n) The total number of counts in the source region in the 0.3-10 keV band (Counts_band0) (phot.count;em.X-ray)
  (1+2+3)Ct1 ct (n) The total number of counts in the source region in the 0.3-1 keV band (Counts_band1) (phot.count;em.X-ray.soft)
  (1+2+3)Ct2 ct (n) The total number of counts in the source region in the 1-2 keV band (Counts_band2) (phot.count;em.X-ray.soft)
  (1+2+3)Ct3 ct (n) The total number of counts in the source region in the 2-10 keV band (Counts_band3) (phot.count;em.X-ray.medium)
  (1+2+3)BgCt0 ct (n) The total number of background counts expected in the source region in 0.3-10 keV band (BgCounts_band0) (phot.count;em.X-ray)
  (1+2+3)BgCt1 ct (n) The total number of background counts expected in the source region in the 0.3-1 keV band (BgCounts_band1) (phot.count;em.X-ray.soft)
  (1+2+3)BgCt2 ct (n) The total number of background counts expected in the source region in the 1-2 keV band (BgCounts_band2) (phot.count;em.X-ray.soft)
  (1+2+3)BgCt3 ct (n) The total number of background counts expected in the source region in the 2-10 keV band (BgCounts_band3) (phot.count;em.X-ray.medium)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)CF0  (n) The PSF correction factor in the 0.3-10 keV band (RateCF_band0) (instr.param)
  (1+2+3)CF1  (n) The PSF correction factor in the 0.3-1 keV band (RateCF_band1) (instr.param)
  (1+2+3)CF2  (n) The PSF correction factor in the 1-2 keV band (RateCF_band2) (instr.param)
  (1+2+3)CF3  (n) The PSF correction factor in the 2-10 keV band (RateCF_band3) (instr.param)
  (1+2+3)FUL0 ct/s (n) The 3-sigma upper confidence limit on the count-rate in the 0.3-10 keV band (UL_band0) (phot.count;arith.rate;em.X-ray)
  (1+2+3)FUL1 ct/s (n) The 3-sigma upper confidence limit on the count-rate in the 0.3-1 keV band (UL_band1) (phot.count;arith.rate;em.X-ray.soft)
  (1+2+3)FUL2 ct/s (n) The 3-sigma upper confidence limit on the count-rate in the 1-2 keV band (UL_band2) (phot.count;arith.rate;em.X-ray.soft)
  (1+2+3)FUL3 ct/s (n) The 3-sigma upper confidence limit on the count-rate in the 2-10 keV band (UL_band3) (phot.count;arith.rate;em.X-ray.medium)
  (1+2+3)PCR0 ct/s (n) The peak count-rate in 0.3-10 keV band (PeakRate_band0) (phot.count;arith.rate;em.X-ray)
  (1+2+3)E_PCR0 ct/s (n) The 1-sigma positive uncertainty on the peak count-rate in the 0.3-10 keV band (PeakRateband0pos) (stat.error;stat.max)
  (1+2+3)e_PCR0 ct/s (n) []? The 1-sigma negative uncertainty on the peak count-rate in 0.3-10 keV band (PeakRateband0neg) (stat.error)
  (1+2+3)PCR1 ct/s (n) The peak count-rate in 0.3-1 keV band (PeakRate_band1) (phot.count;arith.rate;em.X-ray.soft)
  (1+2+3)E_PCR1 ct/s (n) The 1-sigma positive uncertainty on the peak count-rate in the 0.3-1 keV band (PeakRateband1pos) (stat.error;stat.max)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)e_PCR1 ct/s (n) []? The 1-sigma negative uncertainty on the peak count-rate in 0.3-1 keV band (PeakRateband1neg) (stat.error)
  (1+2+3)PCR2 ct/s (n) The peak count-rate in the 1-2 keV band (PeakRate_band2) (phot.count;arith.rate;em.X-ray.soft)
  (1+2+3)E_PCR2 ct/s (n) The 1-sigma positive uncertainty on the peak count-rate in the 1-2 keV band (PeakRateband2pos) (stat.error;stat.max)
  (1+2+3)e_PCR2 ct/s (n) []? The 1-sigma negative uncertainty on the peak count-rate in the 1-2 keV band (PeakRateband2neg) (stat.error)
  (1+2+3)PCR3 ct/s (n) The peak count-rate in the 2-10 keV band (PeakRate_band3) (phot.count;arith.rate;em.X-ray.medium)
  (1+2+3)E_PCR3 ct/s (n) The 1-sigma positive uncertainty on the peak count-rate in the 2-10 keV band (PeakRateband3pos) (stat.error;stat.max)
  (1+2+3)e_PCR3 ct/s (n) []? The 1-sigma negative uncertainty on the peak count-rate in 2-10 keV band (PeakRateband3neg) (stat.error)
  (1+2+3)PcstS0  (n) The probability that the source count-rate in the 0.3-10 keV band does not vary between snapshots (PvarPchiSnapshot_band0) (stat.fit.goodness)
  (1+2+3)PcstS1  (n) The probability that the source count-rate in the 0.3-1 keV band does not vary between snapshots (PvarPchiSnapshot_band1) (stat.fit.goodness)
  (1+2+3)PcstS2  (n) The probability that the source count-rate in the 1-2 keV band does not vary between snapshots (PvarPchiSnapshot_band2) (stat.fit.goodness)
  (1+2+3)PcstS3  (n) The probability that the source count-rate in the 2-10 keV band does not vary between snapshots (PvarPchiSnapshot_band3) (stat.fit.goodness)
  (1+2+3)PcstSHR1  (n) The probability that the source HR1 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR1) (stat.fit.goodness)
  (1+2+3)PcstSHR2  (n) The probability that the source HR2 hardness ratio does not vary between snapshots (PvarPchiSnapshot_HR2) (stat.fit.goodness)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)Pcst0  (n) The probability that the source count-rate in the 0.3-10 keV band does not vary between observations (PvarPchiObsID_band0) (stat.fit.goodness)
  (1+2+3)Pcst1  (n) The probability that the source count-rate in the 0.3-1 keV band does not vary between observations (PvarPchiObsID_band1) (stat.fit.goodness)
  (1+2+3)Pcst2  (n) The probability that the source count-rate in the 1-2 keV band does not vary between observations (PvarPchiObsID_band2) (stat.fit.goodness)
  (1+2+3)Pcst3  (n) The probability that the source count-rate in the 2-10 keV band does not vary between observations (PvarPchiObsID_band3) (stat.fit.goodness)
  (1+2+3)PcstHR1  (n) The probability that the source HR1 hardness ratio does not vary between observations (PvarPchiObsID_HR1) (stat.fit.goodness)
  (1+2+3)PcstHR2  (n) The probability that the source HR2 hardness ratio does not vary between observations (PvarPchiObsID_HR2) (stat.fit.goodness)
  (1+2+3)NHg cm-2 The Galactic absorption column density (in cm-2) in the direction of the source, determined from Willingale et al (2013MNRAS.431..394W) (GalacticNH) (phys)
  (1+2+3)Pow  (n) Which of the available estimates of the power-law spectral ECF and fluxes (WhichPow) (Note 6)   (meta.code)
  (1+2+3)APEC  (n) Which of the available estimates of the APEC spectral ECF and fluxes (WhichAPEC) (Note 7)   (meta.code)
  (1+2+3)CFO0 mJ/m2/ct (n) The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming a power-law spectrum (PowECFO) (instr.param)
  (1+2+3)CFU0 mJ/m2/ct (n) The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming a power-law spectrum (PowECFU) (instr.param)
  (1+2+3)FPO0 mW/m2 (n) The mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FPO0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux_pos) (stat.error;stat.max)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)e_FPO0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming a power-law spectrum (PowFlux_neg) (stat.error)
  (1+2+3)FPU0 mW/m2 (n) The mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FPU0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FPU0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowUnabsFlux_neg) (stat.error)
  (1+2+3)ECFO0 mJ/m2/ct (n) The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming an APEC spectrum (APECECFO) (instr.param)
  (1+2+3)ECFU0 mJ/m2/ct (n) The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming an APEC spectrum (APECECFU) (instr.param)
  (1+2+3)FAO0 mW/m2 (n) The mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FAO0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FAO0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming an APEC spectrum (APECFlux_neg) (stat.error)
  (1+2+3)FAU0 mW/m2 (n) The mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FAU0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FAU0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECUnabsFlux_neg) (stat.error)
  (1+2+3)FpPO0 mW/m2 (n) The peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux) (phot.flux;em.X-ray)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)E_FpPO0 mW/m2 (n) The 1-sigma positive uncertainty on the peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FpPO0 mW/m2 (n) []? The 1-sigma negative uncertainty on the peak 0.3-10 keV observed flux assuming a power-law spectrum (PowPeakFlux_neg) (stat.error)
  (1+2+3)FpPU0 mW/m2 (n) The peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FpPU0 mW/m2 (n) The 1-sigma positive uncertainty on the peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FpPU0 mW/m2 (n) []? The 1-sigma negative uncertainty on the peak 0.3-10 keV unabsorbed flux assuming a power-law spectrum (PowPeakUnabsFlux_neg) (stat.error)
  (1+2+3)FpAO0 mW/m2 (n) The peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FpAO0 mW/m2 (n) The 1-sigma positive uncertainty on the peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FpAO0 mW/m2 (n) []? The 1-sigma negative uncertainty on the peak 0.3-10 keV observed flux assuming an APEC spectrum (APECPeakFlux_neg) (stat.error)
  (1+2+3)FpAU0 mW/m2 (n) The peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FpAU0 mW/m2 (n) The 1-sigma positive uncertainty on the peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FpAU0 mW/m2 (n) []? The 1-sigma negative uncertainty on the peak 0.3-10 keV unabsorbed flux assuming an APEC spectrum (APECPeakUnabsFlux_neg) (stat.error)
  (1+2+3)CECFO mJ/m2/ct (n) 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) (instr.param)
  (1+2+3)CECFU mJ/m2/ct (n) 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) (instr.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)FCOP0 mW/m2 (n) The mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FCOP0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FCOP0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the canned power-law spectrum (FixedPowFlux_neg) (stat.error)
  (1+2+3)FCUP0 mW/m2 (n) The mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FCUP0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FCUP0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned power-law spectrum (FixedPowUnabsFlux_neg) (stat.error)
  (1+2+3)AECFO mJ/m2/ct (n) The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV observed flux, assuming the canned APEC spectrum (FixedAPECECFO) (instr.param)
  (1+2+3)AECFU mJ/m2/ct (n) The Energy Conversion Factor from 0.3-10 keV count-rate to 0.3-10 keV unabsorbed flux, assuming the canned APEC spectrum (FixedAPECECFU) (instr.param)
  (1+2+3)FCAO0 mW/m2 (n) The mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FCAO0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FCAO0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the canned APEC spectrum (FixedAPECFlux_neg) (stat.error)
  (1+2+3)FCAU0 mW/m2 (n) The mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FCAU0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_pos) (stat.error;stat.max)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)e_FCAU0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the canned APEC spectrum (FixedAPECUnabsFlux_neg) (stat.error)
  (1+2+3)PECFO mJ/m2/ct (n) 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) (instr.param)
  (1+2+3)PECFU mJ/m2/ct (n) 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) (instr.param)
  (1+2+3)NH1H cm-2 (n) The hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH) (phys.columnDensity)
  (1+2+3)E_NH1H cm-2 (n) []? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH_pos) (stat.error;stat.max)
  (1+2+3)e_NH1H cm-2 (n) []? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the power-law spectrum interpolated from the HRs (InterpPowNH_neg) (stat.error)
  (1+2+3)Gam  (n) The spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma) (spect.index)
  (1+2+3)E_Gam  (n) []? 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.max)
  (1+2+3)e_Gam  (n) []? The 1-sigma negative uncertainty on the spectral photon index inferred assuming the power-law spectrum interpolated from the HRs (InterpPowGamma_neg) (stat.error)
  (1+2+3)FIPO0 mW/m2 (n) The mean 0.3-10 keV observed flux assuming the power-law spectrum interpolated from the HRs (InterpPowFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FIPO0 mW/m2 (n) 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) (stat.error;stat.max)
  (1+2+3)e_FIPO0 mW/m2 (n) []? 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) (stat.error)
  (1+2+3)FIPU0 mW/m2 (n) The mean 0.3-10 keV unabsorbed flux assuming the power-law spectrum interpolated from the HRs (InterpPowUnabsFlux) (phot.flux;em.X-ray)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)E_FIPU0 mW/m2 (n) 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) (stat.error;stat.max)
  (1+2+3)e_FIPU0 mW/m2 (n) []? 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) (stat.error)
  (1+2+3)IPECFO mJ/m2/ct (n) 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) (instr.param)
  (1+2+3)IPECFU mJ/m2/ct (n) 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) (instr.param)
  (1+2+3)NH2A cm-2 (n) The hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH) (phys.columnDensity)
  (1+2+3)E_NH2A cm-2 (n) []? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_pos) (stat.error;stat.max)
  (1+2+3)e_NH2A cm-2 (n) []? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECNH_neg) (stat.error)
  (1+2+3)kTAH keV (n) The temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT) (phys.temperature)
  (1+2+3)E_kTAH keV (n) []? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT_pos) (stat.error;stat.max)
  (1+2+3)e_kTAH keV (n) []? The 1-sigma negative uncertainty on the temperature inferred assuming the APEC spectrum interpolated from the HRs (InterpAPECkT_neg) (stat.error)
  (1+2+3)FAIO0 mW/m2 (n) The mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FAIO0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FAIO0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV observed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECFlux_neg) (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)FAIU0 mW/m2 (n) The mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FAIU0 mW/m2 (n) The 1-sigma positive uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_pos) (stat.error;stat.max)
  (1+2+3)e_FAIU0 mW/m2 (n) []? The 1-sigma negative uncertainty on the mean 0.3-10 keV unabsorbed flux assuming the APEC spectrum interpolated from the HRs (InterpAPECUnabsFlux_neg) (stat.error)
  (1+2+3)Ppow  (n) 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.goodness)
  (1+2+3)PAPEC  (n) The probability that the HR values of this source could be obtained if the true spectrum is an APEC (P_APEC) (stat.fit.goodness)
  (1+2+3)FPECFO mJ/m2/ct (n) 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) (instr.param)
  (1+2+3)FPECFU mJ/m2/ct (n) 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) (instr.param)
  (1+2+3)NH2C cm-2 (n) The hydrogen column density inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowNH) (phys.columnDensity)
  (1+2+3)E_NH2C cm-2 (n) []? 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) (stat.error;stat.max)
  (1+2+3)e_NH2C cm-2 (n) []? 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) (stat.error)
  (1+2+3+11)Gamma  (n) The spectral photon index inferred assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowGamma) (spect.index)
  (1+2+3)E_Gamma  (n) []? 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.max)
  (1+2+3)e_Gamma  (n) []? 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.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)FPCO0 mW/m2 (n) The mean 0.3-10 keV observed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FPCO0 mW/m2 (n) 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) (stat.error;stat.max)
  (1+2+3)e_FPCO0 mW/m2 (n) []? 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) (stat.error)
  (1+2+3)FPCU0 mW/m2 (n) The mean 0.3-10 keV unabsorbed flux assuming the power-law spectral model fitted to a custom-built spectrum (FittedPowUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FPCU0 mW/m2 (n) 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) (stat.error;stat.max)
  (1+2+3)e_FPCU0 mW/m2 (n) []? 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) (stat.error)
  (1+2+3+7+11)Cstat  (n) The C-statistic from the power-law spectral fit to the custom-built spectrum (FittedPowCstat) (stat.fit.param)
  (1+2+3)DOF  (n) The number of degrees of freedom in the power-law spectral fit to the custom-built spectrum (FittedPowDOF) (meta.number)
  (1+2+3)Chi2r  (n) The Churazov-weighted reduced chi^2 from the power-law spectral fit to the custom-built spectrum (FittedPowReducedChi2) (stat.fit.chi2)
  (1+2+3)ACECFO mJ/m2/ct (n) 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) (stat.fit.goodness)
  (1+2+3)ACECFU mJ/m2/ct (n) 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) (stat.fit.goodness)
  (1+2+3)NH2AC cm-2 (n) The hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH) (phys.columnDensity)
  (1+2+3)E_NH2AC cm-2 (n) []? The 1-sigma positive uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_pos) (stat.error;stat.max)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)e_NH2AC cm-2 (n) []? The 1-sigma negative uncertainty on the hydrogen column density inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECNH_neg) (stat.error)
  (1+2+3)kTAC keV (n) The temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT) (phys.temperature)
  (1+2+3)E_kTAC keV (n) []? The 1-sigma positive uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_pos) (stat.error;stat.max)
  (1+2+3)e_kTAC keV (n) []? The 1-sigma negative uncertainty on the temperature inferred assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECkT_neg) (stat.error)
  (1+2+3)FACO0 mW/m2 (n) The mean 0.3-10 keV observed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FACO0 mW/m2 (n) 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) (stat.error;stat.max)
  (1+2+3)e_FACO0 mW/m2 (n) []? 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) (stat.error)
  (1+2+3)FACU0 mW/m2 (n) The mean 0.3-10 keV unabsorbed flux assuming the APEC spectral model fitted to a custom-built spectrum (FittedAPECUnabsFlux) (phot.flux;em.X-ray)
  (1+2+3)E_FACU0 mW/m2 (n) 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) (stat.error;stat.max)
  (1+2+3)e_FACU0 mW/m2 (n) []? 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) (stat.error)
  (1+2+3)CstatA  (n) The C-statistic from the APEC spectral fit to the custom-built spectrum (FittedAPECCstat) (stat.fit.param)
  (1+2+3)DOFA  (n) The number of degrees of freedom in the APEC spectral fit to the custom-built spectrum (FittedAPECDOF) (meta.number)
  (1+2+3)Chi2rA  (n) The Churazov-weighted reduced chi^2 from the APEC spectral fit to the custom-built spectrum (FittedAPECReducedChi2) (stat.fit.chi2)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)HasSpec  Whether a custom-built spectrum was created for this source (HasSpec) (meta.code)
  (1+2+3)NExt  (n) The number of external sources found to agree spatially with this one at the 3-sigma level (NumExternalMatches) (meta.code)
  (1+2+3)NExt2  (n) 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.code)
  (1+2+3)ROSHRI  Whether the source is spatially within 3 sigma of a source in the Rosat HRI catalogue (Cat. IX/28) (MatchInROSHRI) (meta.code)
  (1+2+3)2RXS  Whether the source is spatially within 3 sigma of a source in the 2RXS catalogue (Cat. J/A+A/588/A103) (MatchIn2RXS) (meta.code)
  (1+2+3)3XMMDR8  Whether the source is spatially within 3 sigma of a source in the 3XMM-DR8 catalogue (Cat. IX/55) (MatchIn4XMM_DR10) (meta.code)
  (1+2+3)3XMMDR7s  Whether the source is spatially within 3 sigma of a source in the 3XMM-DR7s (stacked) catalogue (Cat. IX/56) (MatchIn4XMM_DR10s) (meta.code)
  (1+2+3)XMMSL2  Whether the source is spatially within 3 sigma of a source in the XMMSL2 catalogue (Cat. IX/53) (MatchInXMMSL2) (meta.code)
  (1+2+3)SwiftFT  Whether the source is spatially within 3 sigma of a source in the SwiftFT catalog (Cat. J/A+A/528/A122) (MatchInSwiftFT) (meta.code)
  (1+2+3)1SWXRT  Whether the source is spatially within 3 sigma of a source in the 1SWXRT catalogue (Cat. J/A+A/551/A142) (MatchIn1SWXRT) (meta.code)
  (1+2+3)XRTGRB  Whether the source is spatially within 3 sigma of an XRT GRB afterglow (MatchInXRTGRB) (meta.code)
  (1+2+3)SDSSQSO  Whether the source is spatially within 3 sigma of a source in the SDSS QSO DR14 catalogue (MatchInSDSSQSODR14) (meta.code)
  (1+2+3)2MASS  Whether the source is spatially within 3 sigma of a source in the 2MASS catalogue (Cat. II/246) (MatchIn2MASS) (meta.code)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3)USNOB1  Whether the source is spatially within 3 sigma of a source in the USNO-B1 catalogue (Cat. I/284) (MatchInUSNOB1) (meta.code)
  (1+2+3)2CSC  Whether the source is spatially within 3 sigma of a source in the 2CSC catalogue (MatchIn2CSC) (meta.code)
  (1+2+3)2SXPS  Whether the source is spatially within 3 sigma of a source in the 2SXPS (Cat. IX/58) catalogue (MatchIn2SXPS) (meta.code)
  (4+5+6+7+8+10)DataID  The unique identifier for this dataset (DatasetID) (meta.id)
  (4+5+6+7+10)ObsID  The identifier of the observation or stacked image in which this detection occurred (ObsID) (meta.id;meta.main)
  (4+5+6)Version  The version of this dataset (DataVersion) (Note 1)   (meta.version;meta.dataset)
  (4+5+6)Stacked  Whether or not this is a stacked image (IsStackedImage) (meta.code)
  (4+5+6)FFlag  The warning flag associated with this dataset (FieldFlag) (Note 2)   (meta.code)
  (4+5+6)Size  The side length of the field image in XRT pixels (2.357 arcsec per pixel) (ImageSize) (phys.size;obs.field)
  (4+5+6+8)Exp s The nominal exposure in the dataset, after all screening has been carried out (ExposureUsed) (meta.dataset;obs.exposure)
  (4+5+6)OExp s The original nominal exposure in the dataset before screening (OriginalExposure) (meta.dataset;obs.exposure)
  (4+5+6)time.mid1 s The mid-time of the dataset, in Swift Mission Elapsed Time (MidTime_MET) (time.epoch)
  (4+5+6)time.mid2 s The mid-time of the dataset, in Barycentric Dynamical Time (MidTime_TDB) (time.epoch)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4+5+6)time.mid3 s The mid-time of the dataset, as a Modified Julian Date (MidTime_MJD) (time.epoch)
  (4+5+6+10)LiveDate s (n)(i) The UTC date at which this dataset became live (LiveDate) (time.epoch)
  (4+5+6)FBGb0 ct/pix/s The mean background level in the 0.3-10 keV band (FieldBG_band0) (instr.background;em.X-ray.medium;stat.mean)
  (4+5+6)FBGb1 ct/pix/s The mean background level in the 0.3-1 keV band (FieldBG_band1) (instr.background;em.X-ray.soft;stat.mean)
  (4+5+6)FBGb2 ct/pix/s The mean background level in the 1-2 keV band (FieldBG_band2) (instr.background;em.X-ray.soft;stat.mean)
  (4+5+6)FBGb3 ct/pix/s The mean background level in the 2-10 keV band (FieldBG_band3) (instr.background;em.X-ray.medium;stat.mean)
  (4+5+6)Nbr0  The number of sources detected in this dataset in the 0.3-10 keV band (NumSrc_band0) (meta.number)
  (4+5+6)NOK0  The number of good or reasonable sources detected in this dataset in the 0.3-10 keV band (NumOK_band0) (meta.number)
  (4+5+6)MD0 pc (n) The median distance between sources detected in this dataset in the 0.3-10 keV band (MedianDist_band0) (pos.distance)
  (4+5+6)Nbr1  The number of sources detected in this dataset in the 0.3-1 keV band (NumSrc_band1) (meta.number)
  (4+5+6)NOK1  The number of good or reasonable sources detected in this dataset in the 0.3-1 keV band (NumOK_band1) (meta.number)
  (4+5+6)MD1 pc (n) The median distance between sources detected in this dataset in the 0.3-1 keV band (MedianDist_band1) (pos.distance)
  (4+5+6)Nbr2  The number of sources detected in this dataset in the 1-2 keV band (NumSrc_band2) (meta.number)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4+5+6)NOK2  The number of good or reasonable sources detected in this dataset in the 1-2 keV band (NumOK_band2) (meta.number)
  (4+5+6)MD2 pc (n) The median distance between sources detected in this dataset in the 1-2 keV band (MedianDist_band2) (pos.distance)
  (4+5+6)Nbr3  The number of sources detected in this dataset in the 2-10 keV band (NumSrc_band3) (meta.number)
  (4+5+6)NOK3  The number of good or reasonable sources detected in this dataset in the 2-10 keV band (NumOK_band3) (meta.number)
  (4+5+6)MD3 pc (n) The median distance between sources detected in this dataset in the 2-10 keV band (MedianDist_band3) (pos.distance)
  (4+5+6)NSnaps  The number of snapshots contributing to this dataset (NumberOfSnapshots) (meta.number)
  (4+5+6)ErrAst arcsec (n) The 90% confidence radial uncertainty on the XRT-2MASS astrometric correction (AstromError) (stat.error)
  (4+5+6)CRV1c  (n) The CRVAL1 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CRVAL1_corr) (instr.param)
  (4+5+6)CRV2c  (n) The CRVAL2 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CRVAL2_corr) (instr.param)
  (4+5+6)CROT2c  (n) The CROTA1 WCS reference value for the dataset derived from the XRT-2MASS astrometric correction (CROTA2_corr) (instr.param)
  (4+5+6)Stack  Whether 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.code)
  (7+8)DetID  A unique identifier for this detection (DetectionID) (meta.id;meta.main)
  (7+8+11)ObsSID  (i) The ID of the obsSource this detection is part of (ObsSourceID) (meta.id)

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  (7)Obs (char) Link to obsource (meta.ref.url)
  (7)SNo  The identifier of this source within this obsid and band (SourceNo) (meta.id)
  (7)Band  The band in which this detection occurred (Band) (Note 1)   (instr.bandpass)
  (7)ExpCor s The exposure time at the position of the source in this obsID (CorrectedExposure) (time.duration;obs.exposure)
  (7)ExpFrac s The fractional exposure at the position of this source, i.e. the exposure divided by the nominal exposure for the field (ExposureFraction) (time.expo)
  (7)E_RAJ2000 deg The 1-sigma positive uncertainty on the right ascension (RA_pos) (stat.error;stat.max)
  (7)e_RAJ2000 deg The 1-sigma negative uncertainty on the right ascension (RA_neg) (stat.error;pos.eq.ra)
  (7)E_DEJ2000 deg The 1-sigma positive uncertainty on the declination (Decl_pos) (stat.error;stat.max)
  (7)e_DEJ2000 deg The 1-sigma negative uncertainty on the declination (Decl_neg) (stat.error;pos.eq.dec)
  (7)RAcordeg deg (n) Right Ascension corrected using XRT-2MASS astrometry (J2000) (RA_corrected) (pos.eq.ra)
  (7)DEcordeg deg (n) Declination corrected using XRT-2MASS astrometry (J2000) (Decl_corrected) (pos.eq.dec)
  (7)Err90corr arcsec (n) Uncertainty on the corrected position, 90% confidence, radial, assumed to be Rayleigh-distributed (Err90_corrected) (stat.error;pos)
  (7)GLONcor deg (n) Galactic longitude corrected using XRT-2MASS astrometry (l_corrected) (pos.galactic.lon)

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  (7)GLATcor deg (n) Galactic latitude corrected using XRT-2MASS astrometry (b_corrected) (pos.galactic.lat)
  (7)X pix The x position of the object in the SKY image plane (IMG_X) (pos.cartesian.x;instr.plate)
  (7)Y pix The y position of the object in the SKY image plane (IMG_Y) (pos.cartesian.y;instr.plate)
  (7)DetFlag  The best detection flag from all detections of the source (DetFlag) (Note 2)   (meta.code)
  (7)MatchX  Whether the position of this source matches a known extended X-ray source (MatchesKnownExtended) (meta.code)
  (7)Pileup  Whether the accepted fit included pile up (PileupFitted) (meta.code)
  (7)SNR  The signal to noise ratio of the detection (SNR) (stat.snr)
  (7)CtsPSF ct Number of counts in the image region over which the final PSF fit was performed (CtsInPSFFit) (phot.count;em.X-ray)
  (7)BGPSF ct/s Mean count-rate in the background map in the region over which the final PSF fit was performed (BGRateInPSFFit) (phot.count;em.X-ray)
  (7)CstatNo  The C-statistic value derived over the PSF fit region if no source is fitted (Cstat_nosrc) (stat.fit.param)
  (7)Lsrc  The log-likelihood value that this detection is not just a background fluctuation (L_src) (stat.likelihood)
  (7)CstatF  The 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.param)
  (7)LFlat  The log-likelihood value that this detection is PSF like, not a flat count increase (Lflat) (stat.likelihood)

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  (7)FracPix  The fraction of pixels within the PSF fit region which are exposed (FracPix) (instr.saturation)
  (7)PileS  The best-fitting S parameter of the pile-up model, if fitted (Pileup_S) (stat.fit.param)
  (7)Pilel  The best-fitting l parameter of the pile-up model, if fitted (Pileup_l) (stat.fit.param)
  (7)Pilec  The best-fitting c parameter of the pile-up model, if fitted (Pileup_c) (stat.fit.param)
  (7)Piletau  The best-fitting tau parameter of the pile-up model, if fitted (Pileup_tau) (stat.fit.param)
  (7)CstatPile  The 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.param)
  (7)PSFRad  The radius of the circular region over which PSF fitting was carried out (in image pixels, 2.357"" to a side) (PSFFitRadius) (instr.det.psf;obs.field)
  (7)BoxWidth  The 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.width)
  (7)Rate ct/s The corrected count-rate of this detection (i.e. in the band of this image) (Rate) (phot.count;em.X-ray)
  (7)E_Rate ct/s The 1-sigma positive uncertainty on the count rate (Rate_pos) (stat.error;stat.max)
  (7)e_Rate ct/s The 1-sigma negative uncertainty on the count rate (Rate_neg) (stat.error)
  (7)Cts ct The total number of counts in the region used to extract the count rate (CtsInRate) (phot.count;em.X-ray)
  (7)BGCts ct The total number of counts in the region used to extract the count rate (BGCtsInRate) (phot.count;em.X-ray)

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  (7)CF  The PSF correction factor for the count rate (Rate_CF) (instr.param)
  (7)BGRate ct/s The background rate in the region used for count-rate calculation (BGRateInRate) (phot.count;em.X-ray)
  (8)OSNum  The identifier of this obsSource within this dataset (OSNum) (meta.id)
  (8)CorPos  Whether or not the astrometrically-corrected position of this obsSource should be used (UsedCorrectedPosition) (meta.code)
  (8)BBand  The energy band corresponding to the best detection of this obsSource in this dataset (BestBand) (instr.bandpass)
  (8)Pile  (n) 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.code)
  (8)Orphan  Whether this source is one which is only detected in this dataset, and this dataset is deprecated (IsOrphanSource) (meta.code)
  (9)ExtCat (char) The catalogued name of the external source (ExtCat_ID) (meta.id.assoc)
  (9)Cat (char) The catalogue in which the external source was found (Catalogue) (meta.id;meta.dataset)
  (9)D arcsec The distance between the 2SXPS and external source positions (Distance) (pos.angDistance)
  (9)ExtRA deg (i) The right ascension of the external source (J2000) (Ext_RA) (pos.eq.ra;meta.main)
  (9)ExtDE deg (i) The declination of the external source (J2000) (Ext_Decl) (pos.eq.dec;meta.main)
  (9)ExtErr90 arcsec (n) The 90% confidence radial position error of the external source (Ext_Err90) (Note 1)   (stat.error)

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  (10)DataV  The version of this dataset (DataVersion) (Note 1)   (meta.software)
  (10)Obsolete  Whether 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.code)
  (11)TrsID  A unique numerical identifier for this transient within this catalogue (TransientID) (meta.id;meta.main)
  (11)LSXPSN (char) The IAU name of this object in the main LSXPS catalogue (LSXPSName) (meta.id)
  (11)Class  A numerical code describing how this transient has been classified e.g 64 cases of 1 as confirmed transient (Classification) (meta.code)
  (11)Discovery  The date of the observation in ident number in which the transient was first found (DiscoveryDatasetID) (meta.number)
  (11)PRate ct/s The peak count-rate in the 0.3-10 keV band in the dataset in which the transient was first detected (PeakRateAtDetection) (phot.count;em.X-ray)
  (11)E_PRate ct/s The 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) (stat.error;stat.max)
  (11)e_PRate ct/s The 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) (stat.error)
  (11)PSMRate ct/s The peak count-rate in the 0.3-2 keV band in the dataset in which the transient was first detected (PeakSoftMedBandRateAtDetection) (phot.count;em.X-ray.soft)
  (11)UpperC (char) Where the 'best' upper limit at the source location was taken from, where the 'canned' spectrum is used to convert between observatories (UpperLimitSource_Canned) (meta.note)
  (11)UpperDS (char) Where the 'best' upper limit at the source location was taken from, where the discovery spectrum is used to convert between observatories (UpperLimitSource_DS) (meta.note)
  (11)UpperFS (char) Where the 'best' upper limit at the source location was taken from, where the full spectrum is used to convert between observatories (UpperLimitSource_FS) (meta.note)

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  (11)Sig  How far above the best upper limit the peak count rate is, in Gaussian sigmas (Significance) (arith.rate;phot.count;stat.max)
  (11)NH cm-2 (n) The hydrogen column density found in an automated power-law fit to a spectrum built from the discovery dataset (InitSpecNH) (phys.columnDensity;meta.modelled)
  (11)Chi2  (n) The Churazov-weighted reduced chi^2 from an automated power-law fit to a spectrum built from the discovery dataset (InitSpecTestStat) (stat.fit.chi2)
  (11)Dof  (n) The number of degrees of freedom in the automated power-law fit to a spectrum built from the discovery dataset (InitSpecDof) (meta.number)
  (11)NHFS cm-2 (n) 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) (phys.columnDensity;meta.modelled)
  (11)GammaFS  (n) 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.index)
  (11)CstatFS  (n) 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.param)
  (11)Chi2FS  (n) 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.chi2)
  (11)DofFS  (n) 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.number)
  (11)DiscDate s (n) The date of the analysis in which the transient was first found (DiscoveryDate) (time.epoch)
  (11)DetDate yr (n) The date of the start of the observation in which the transient was first found (DetectionDate) (time.epoch)
  (11)DetMET s The MET of the start of the observation in which the transient was first found (DetectionMET) (time.epoch)
  (11)LSXPSul ct/s (n) An upper limit at the transient derived from the LSXPS catalogue (LSXPS_UpperLimit) (phot.count;em.X-ray)

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  (11)LSXPSulID  (n) The observation in the LSXPS catalogue from which the upper limit was derived (LSXPSUpperLimitObsID) (meta.number)
  (11)XMMul ct/s (n) An XMM-Newton upper limit at the transient location, obtained via the HILIGT server, in native XMM count-rate units (XMMUpperLimitnative) (phot.count;em.X-ray)
  (11)XMMulMode (char) The mode in which XMM was observing when the upper limit was obtained (XMMUpperLimitObsMode) (meta.code)
  (11)XMMulInst (char) The XMM-Newton instrument from which the upper limit was obtained (XMMUpperLimitInstrument) (meta.code)
  (11)XMMulXRTds ct/s (n) 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 (XMMUpperLimitasXRTTotal_DS) (phot.count;em.X-ray)
  (11)XMMulXRTfs ct/s (n) 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 (XMMULasXRTTot_FS) (phot.count;em.X-ray)
  (11)XMMulXRTc ct/s (n) The XMM-Newton upper limit converted to a 0.3-10 keV XRT count rate, using a standard AGN spectrum (XMMUpperLimitasXRTTotal_Canned) (phot.count;em.X-ray)
  (11)RSul ct/s An ROSAT All-Sky Survey upper limit at the transient location, obtained via the HILIGT server, in native ROSAT PSPC count-rate units (RASSUpperLimnative) (phot.count;em.X-ray)
  (11)RSulXRTsmds ct/s (n) 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 (RASSUpperLimitasXRTSoftMed_DS) (phot.count;em.X-ray)
  (11)RSulXRTsmfs ct/s (n) 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 (RASSUpperLimitasXRTSoftMed_FS) (phot.count;em.X-ray)
  (11)RSulXRTsmc ct/s The RASS upper limit converted to a 0.3-2 keV XRT count rate, using a standard AGN spectrum (RASSUpperLimitasXRTSoftMed_Canned) (phot.count;em.X-ray)
  (11)RSulXRTds ct/s (n) 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 (RASSUpperLimitasXRTTotal _DS) (phot.count;em.X-ray)
  (11)RSulXRTfs ct/s (n) 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 (RASSUpperLimitasXRTTotal_FS) (phot.count;em.X-ray)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (11)RSulXRTc ct/s (n) The RASS upper limit converted to a 0.3-10 keV XRT count rate, using a standard AGN spectrum (RASSUpperLimitasXRTTotal_Canned) (phot.count;em.X-ray)
  (11)Notes (char) Any notes added by the XRT team (Notes) (meta.note)

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