J/ApJS/261/32ivo://CDS.VizieR/J/ApJS/261/32doi:10.26093/cds/vizier.22610032CDSFu Y.Wu X.-B.Jiang L.Zhang Y.Huo Z.-Y.Ai Y.L.Yang Q.Ma Q.,Feng X.Joshi R.Hon W.J.Wolf C.Li J.-T.Jin J.-J.Yao SuPang Y.,Wang J.-G.Lu K.-X.Wang C.-J.Zheng J.Xu L.Yu X.-G.Lun B.-L.,Zuo P.2022-11-02T06:45:20Z2022-10-28T12:38:37ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frquasarsgalaxy-planesmilky-way-galaxyredshiftedvisible-astronomyspectroscopyinfrared-photometryphotometryblack-holesline-intensitiesQuasars behind the Galactic plane (GPQs) are important astrometric references and valuable probes of Galactic gas, yet the search for GPQs is difficult due to severe extinction and source crowding in the Galactic plane. In this paper, we present a sample of 204 spectroscopically confirmed GPQs at |b|<20{deg}, 191 of which are new discoveries. This GPQ sample covers a wide redshift range from 0.069 to 4.487. For the subset of 230 observed GPQ candidates, the lower limit of the purity of quasars is 85.2%, and the lower limit of the fraction of stellar contaminants is 6.1%. Using a multicomponent spectral fitting, we measure the emission line and continuum flux of the GPQs, and estimate their single-epoch virial black hole masses. Due to selection effects raised from Galactic extinction and target magnitude, these GPQs have higher black hole masses and continuum luminosities in comparison to the SDSS DR7 quasar sample. The spectral-fitting results and black hole mass estimates are compiled into a main spectral catalog, and an extended spectral catalog of GPQs. The successful identifications prove the reliability of both our GPQ selection methods and the GPQ candidate catalog, shedding light on the astrometric and astrophysical programs that make use of a large sample of GPQs in the future.2022ApJS..261...32Fhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/261/32CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)I/323 : International Celestial Reference Frame 2, ICRF2 (Ma+, 2009)II/328 : AllWISE Data Release (Cutri+ 2013)V/146 : LAMOST DR1 catalogs (Luo+, 2015)II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)J/AJ/131/2766 : Quasar luminosity function from SDSS-DR3 (Richards+, 2006)J/ApJS/165/1 : BAL QSOs from SDSS DR3 (Trump+, 2006)J/ApJ/701/508 : 5000 AGNs behind the Magellanic clouds (Kozlowski+, 2009)J/ApJS/180/67 : Phot. selection of quasars from SDSS. II. (Richards+, 2009)J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)J/A+A/542/A110 : Neutral gas in the Milky Way halo (Ben Bekhti+, 2012)J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012)J/AJ/145/159 : LAMOST. II. ugriz photometry of 526 new quasars (Huo+, 2013)J/other/RAA/15.1438 : LAMOST new QSOs in M31 and M33 vicinity (Huo+, 2015)J/ApJ/825/126 : SEAMBHs. V. The third year (Du+, 2016)J/ApJS/241/34 : The SDSS Reverberation Mapping (SDSS-RM) project (Shen+, 2019)J/ApJS/249/17 : SDSS QSO DR14 spectral properties (Rakshit+, 2020)J/ApJS/254/6 : Finding QSOs behind the Galactic Plane. I. (Fu+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/261/32https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/261/32http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/261/32https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/261/32https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/261/32http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/261/32GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/261/32/gpqcat (Main (Table A1) and extended (Table A2) spectral catalog of the 204 identified quasars behind the Galactic plane (GPQs))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/261/32/gpqcat?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/261/32/gpqcat?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/261/32/gpqcat?GETtext/xml+votable180.050000true0.36434130946.3608386980.005555555555555556Cone search capability for table J/ApJS/261/32/tablec1 (List of the stellar and galaxy contaminants)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/261/32/tablec1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/261/32/tablec1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/261/32/tablec1?GETtext/xml+votable180.050000true2.320024260.20351060.0055555555555555566/1010 1021 1113 1284 1287 1310 1325 1342 1352 1362 1369 1393 1407 1409 1468 1494 1518 1685 1709 1814 1857 1859-1860 1919 2044 2415 2418 2453 2493 2496 2510 2528 2548-2550 2555-2556 2682 2747 2796 2830 2893 2906 2913 2925 2966 2981 2987 2994 3048 3091 3097 3111 3229 3232 3244-3245 3310 3331 3439-3440 3568 3910 3937 6303 6311 6734 6867 12430 12804 12855 12906 12930 13249 13255 13496 13500 13931 13969 14095 14107 14115-14116 14120 14125 14132-14133 14149 14161 14177 14223 14488 14517 14535 14552 14556 14561 14565 14577 14580 14754 14816 14892 15902 15909 20762 20782-20783 21250 21572 21574 21592 21616 21723 21727 21753 21764 21783 21791 21802 21808 21910 21936-21937 21954-21955 22102 22253 22259 22286 22308 22310 22319 22342 22377 22392 22403 22417 22419 22424 22441 22449 22451 22471 22484 22980 22997 23027-23028 23033 23389 23742 23758 23767 23789 23800 23824 23828 23830-23832 23837-23839 23859 23861 23874 23880 23900 23910 23913-23914 24002 24006 24008 24013 24032 24165 24179 24187 24436 24447 24458 24460 24479 29010 29697 29951 30141 30179 30467 31188 31856 31974 31991 31996 32253 32516 32579 32591 40094-40095 40510 40563 40593 40640 40680 40873 40882 40891 42868 42873 48044 48058 48063https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/261/32?format=asciiOpticalInfrareddefaultJ/ApJS/261/32/gpqcatMain (Table A1) and extended (Table A2) spectral catalog of the 204 identified quasars behind the Galactic plane (GPQs)e_FbHa[33.9/11765]? Measurement error in FbHa1e-20W.m**-2stat.errordoublenullablee_EWSII6732[0.7/25]? Measurement error in EWSII67320.1nmstat.errordoublenullableFSII6732[33/516]? Flux of [SII]MgII6732, 10^-17^erg/s/cm21e-20W.m**-2phot.fluxfloatnullablee_FSII6732[5/283]? Measurement error in FSII67321e-20W.m**-2stat.errorfloatnullable_RA.icrsRight ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)degpos.eq.ranullableindexed_DE.icrsDeclination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)degpos.eq.decnullableindexedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameDesignation (JHHMMSS.ss+DDMMSS.s based on PS1) (G1)meta.id;meta.maincharGLON[6.8/355] Galactic longitudedegpos.galactic.lonGLAT[-19.9/19.9] Galactic latitudedegpos.galactic.latimag[15.51/19.91] Mean PSF AB magnitude from PS1 i-filter detectionsmagphot.mag;em.opt.Ifloatz[0.068/4.5] Redshift from visual inspectionsrc.redshiftdoublelogL1350[46.16/48.01]? Log, continuum luminosity at rest-frame 1350{AA}, in erg/s units (G3)log(1e-07W)phys.luminosity;spect.continuumdoublenullablee_logL1350[0.002/0.04]? Measurement error in logL1350 (G3)log(1e-07W)stat.errordoublenullablelogL3000[44.8/48.41]? Log, continuum luminosity at rest-frame 3000{AA}, erg/slog(1e-07W)phys.luminosity;spect.continuum;em.optdoublenullablee_logL3000[0.001/0.06]? Measurement error in logL3000log(1e-07W)stat.errordoublenullablelogL5100[42.88/46]? Log, continuum luminosity at rest-frame 5100{AA}, erg/slog(1e-07W)phys.luminosity;spect.continuum;em.optdoublenullablee_logL5100[0.002/0.04]? Measurement error in logL5100log(1e-07W)stat.errordoublenullablelogBHHb[7.3/9.4]? Log, single-epoch virial BH mass based on H{beta}log(solMass)phys.massdoublenullablee_logBHHb[0.012/0.5]? Uncertainty in logBH-HBlog(solMass)stat.errordoublenullablelogBHMgII[8.13/10.62]? Log, single-epoch virial BH mass based on MgIIlog(solMass)phys.massdoublenullablee_logBHMgII[0.0009/0.64]? Uncertainty in logBHMgIIlog(solMass)stat.errordoublenullablelogBHCIV[9.1/10.52]? Log, single-epoch virial BH mass based on CIV (G3)log(solMass)phys.massdoublenullablee_logBHCIV[0.025/0.34]? Uncertainty in logBHCIV (G3)log(solMass)stat.errordoublenullableTelTelescope used to acquire the spectrum (G4)instr.setupcharRAdegPS1 Right Ascension (J2000) (G2)degpos.eq.ra;meta.mainDEdegPS1 Declination (J2000) (G2)degpos.eq.dec;meta.mainEBV[0.029/0.7] Line-of-sight E(B-V) given by the Planck (2014A&A...571A..11P) dust mapphot.color.excessfloatiMAG2[-31/-21] SDSS i-band absolute magnitude M_i(z=2), K-corrected to z=2magphys.magAbs;em.opt.IdoubleMJD[58252.77/59345.88] Modified Julian Date of spectroscopic observation (JD-2400000.5)dtime.epochdoubleSNRSp[1.4/41] Median S/N per pixel of the spectrumstat.snr;stat.medianfloatFenormUV[0.07/239]? Normalization factor of the ultraviolet FeII templatearith.factorfloatnullableFeShiftUV[-0.01/0.01]? Wavelength shift of the ultraviolet FeII templateem.wl;arith.diffdoublenullableFeFWHMUV[1200/10000]? Gaussian FWHM applied to convolve the ultraviolet FeIIarith.factordoublenullableFenormOp[0.38/755]? Normalization factor of the optical FeII templatearith.factor;em.optfloatnullableFeShiftOp[-0.01/0.01]? Wavelength shift of the optical FeII templateem.wl;arith.diffdoublenullableFeFWHMOp[1200/10000]? Gaussian FWHM applied to convolve the optical FeII templatearith.factor;em.optdoublenullablePLnorm[0.06/10397]? Normalization factor of the power-law model, in 10^-17^erg/s/cm2/{AA}1e-17cW.m**-2.nm**-1arith.factor;meta.modelleddoublenullablePLalpha[-5/3]? Wavelength power-law indexspect.indexfloatnullablePolyA[-4.2/4.8]? Efficient of the three-order polynomial model (b1)stat.fit.paramdoublenullablePolyB[-0.007/0.004]? Efficient of the three-order polynomial model (b2)stat.fit.paramdoublenullablePolyC[-3.4e-7/3.3e-6]? Efficient of the three-order polynomial model (b3)stat.fit.paramdoublenullableNpixCIV[134/946]? Number of good pixels for the rest-frame 1500-1700{AA}meta.numberfloatnullableStCIV[1/5]? Line-fitting status of CIVmeta.codefloatnullableSNCIV[1.6/33.4]? Median S/N per pixel for the rest-frame 1500-1700{AA}stat.snr;stat.medianfloatnullableFWHMCIV[3135/13615]? FWHM of the whole CIVkm/sspect.line.widthdoublenullablee_FWHMCIV[148/3100]? Measurement error in FWHMCIVkm/sstat.errorfloatnullableEWCIV[10/91]? Rest-frame equivalent width of the whole CIV0.1nmspect.line.eqWidthdoublenullablee_EWCIV[0.4/12]? Measurement error in EWCIV0.1nmstat.errordoublenullableFCIV[259/789498]? FLUX of the whole CIV, 10-^17^erg/s/cm21e-20W.m**-2phot.fluxdoublenullablee_FCIV[17/47653]? Measurement error in FCIV1e-20W.m**-2stat.errordoublenullableNpixCIII[56/1159]? Number of good pixels for the rest-frame 1700-1970{AA}meta.numberfloatnullableStCIII[1/2]? Line-fitting status of CIIImeta.codefloatnullableSNCIII[0.29/35]? Median S/N per pixel for the rest-frame 1700-1970{AA}stat.snr;stat.medianfloatnullableFWHMCIII[2826/14449]? FWHM of the whole CIIIkm/sspect.line.widthdoublenullablee_FWHMCIII[48/4223]? Measurement error in FWHMCIIIkm/sstat.errorfloatnullableEWCIII[2/71]? Rest-frame equivalent width of the whole CIII0.1nmspect.line.eqWidthdoublenullablee_EWCIII[0.36/8.6]? Measurement error in EWCIII0.1nmstat.errordoublenullableFCIII[148/254655]? FLUX of the whole CIII, 10^-17^erg/s/cm21e-20W.m**-2phot.fluxdoublenullablee_FCIII[26/16181]? Measurement error in FCIII1e-20W.m**-2stat.errordoublenullableNpixMgII[47/730]? Number of good pixels for the rest-frame 2700-2900{AA}meta.numberfloatnullableStMgII[1/5]? Line-fitting status of MgIImeta.codefloatnullableSNMedMgII[0.5/42]? Median S/N per pixel for the rest-frame 2700-2900{AA}stat.snr;stat.medianfloatnullableFWHMbMgII[1622/10609]? FWHM of the whole broad MgIIkm/sspect.line.widthdoublenullablee_FWHMbMgII[12/2826]? Measurement error in FWHMbMgIIkm/sstat.errorfloatnullableEWbMgII[8/107]? Rest-frame equivalent width of the whole broad MgII0.1nmspect.line.eqWidthdoublenullablee_EWbMgII[0.4/5.4]? Measurement error in EWbMgII0.1nmstat.errordoublenullableFbMgII[306/403613]? Flux of the whole broad MgII, 10^-17^erg/s/cm21e-20W.m**-2phot.fluxdoublenullablee_FbMgII[21/38994]? Measurement error in FbMgII1e-20W.m**-2stat.errordoublenullableFWHMnMgII[351/1206]? FWHM of Narrow MgIIkm/sspect.line.widthfloatnullablee_FWHMnMgII[0.007/407]? Measurement error in FWHMnMgIIkm/sstat.errorfloatnullableEWnMgII[0.0016/9.42]? Rest-frame equivalent width of Narrow MgII0.1nmspect.line.eqWidthdoublenullablee_EWnMgII[0.08/4]? Measurement error in EWnMgII0.1nmstat.errordoublenullableFnMgII[0.39/5375]? Flux of Narrow MgII, 10^-17^erg/s/cm21e-20W.m**-2phot.fluxfloatnullablee_FnMgII[5/8513]? Measurement error in FnMgII1e-20W.m**-2stat.errorfloatnullableNpixHb[140/1065]? Number of good pixels for the rest-frame 4640-5100{AA}meta.numberfloatnullableStHb[1/5]? Line-fitting status of 4640-5100{AA}meta.codefloatnullableSNMedHb[3.7/43.2]? Median S/N per pixel for the res t-frame 4640-5100{AA}stat.snr;stat.medianfloatnullableFWHMbHb[2826/15493]? FWHM of broad Hbetakm/sspect.line.widthdoublenullablee_FWHMbHb[33/3623]? Measurement error in FWHMbHbkm/sstat.errorfloatnullableEWbHb[6/361]? Rest-frame equivalent width of broad Hbeta0.1nmspect.line.eqWidthdoublenullablee_EWbHb[1/39]? Measurement error in EWbHb0.1nmstat.errordoublenullableFbHb[100/135788]? Flux of broad Hbeta, 10-17erg/s/cm21e-20W.m**-2phot.flux;spect.line;em.line.Hbetadoublenullablee_FbHb[43/25315]? Measurement error in FbHb1e-20W.m**-2stat.errordoublenullableFWHMnHb[168/1204]? FWHM of narrow Hbetakm/sspect.line.widthfloatnullablee_FWHMnHb[14/371]? Measurement error in FWHMnHbkm/sstat.errorfloatnullableEWnHb[0.28/37]? Rest-frame equivalent width of narrow Hbeta0.1nmspect.line.eqWidthdoublenullablee_EWnHb[0.19/9]? Measurement error in EWnHb0.1nmstat.errordoublenullableFnHb[4/7991]? Flux of narrow Hbeta, 10-17erg/s/cm21e-20W.m**-2phot.flux;spect.line;em.line.Hbetafloatnullablee_FnHb[11.9/2879]? Measurement error in FnHb1e-20W.m**-2stat.errorfloatnullableFWHMOIII4959[258.9/2284]? FWHM of [OIII]MgII4959km/sspect.line.widthfloatnullablee_FWHMOIII4959[0.78/767]? Measurement error in FWHMOIII4959km/sstat.errorfloatnullableEWOIII4959[0.6/42]? Rest-frame equivalent width of [OIII]MgII49590.1nmspect.line.eqWidthdoublenullablee_EWOIII4959[0.2/8]? Measurement error in EWOIII49590.1nmstat.errordoublenullableFOIII4959[14.8/3551]? Flux of [OIII]MgII4959, 10^-17^erg/s/cm21e-20W.m**-2phot.fluxfloatnullablee_FOIII4959[11/2439]? Measurement error in FOIII49591e-20W.m**-2stat.errorfloatnullableFWHMOIII5007[336/1954]? FWHM of [OIII]MgII5007km/sspect.line.widthfloatnullablee_FWHMOIII5007[0.7/694]? Measurement error in FWHMOIII5007km/sstat.errorfloatnullableEWOIII5007[1/21152]? Rest-frame equivalent width of [OIII]MgII50070.1nmspect.line.eqWidthdoublenullablee_EWOIII5007[0.2/23816586]? Measurement error in EWOIII50070.1nmstat.errordoublenullableFOIII5007[10/371363]? Flux of [OIII]MgII5007, 10-17erg/s/cm21e-20W.m**-2phot.fluxdoublenullablee_FOIII5007[10/415655263]? Measurement error in FOIII50071e-20W.m**-2stat.errordoublenullableNpixHa[138/421]? Number of good pixels for the rest-frame 6400-6800{AA}meta.numberfloatnullableStHa[1/5]? Line-fitting status of H{alpha}meta.codefloatnullableSNMedHa[7.5/36]? Median S/N per pixel for the rest-frame 6400-6800{AA}stat.snr;stat.medianfloatnullableFWHMbHa[2820/10166]? FWHM of broad H{alpha}km/sspect.line.widthdoublenullablee_FWHMbHa[231/984]? Measurement error in FWHMbHakm/sstat.errorfloatnullableEWbHa[16.8/2578644]? Rest-frame equivalent width of broad H{alpha}0.1nmspect.line.eqWidthdoublenullablee_EWbHa[9/557576]? Measurement error in EWbHa0.1nmstat.errordoublenullableFbHa[82/57519]? Flux of broad H{alpha}, 10-17erg/s/cm21e-20W.m**-2phot.flux;spect.line;em.line.HalphadoublenullableFWHMnHa[353/1205]? FWHM of narrow H{alpha}km/sspect.line.widthfloatnullablee_FWHMnHa[0.14/349]? Measurement error in FWHMnHakm/sstat.errorfloatnullableEWnHa[0.59/51230]? Rest-frame equivalent width of narrow H{alpha}0.1nmspect.line.eqWidthdoublenullablee_EWnHa[4.8/481024]? Measurement error in EWnHa0.1nmstat.errordoublenullableFnHa[22/47532]? Flux of narrow H{alpha}, 10-17erg/s/cm21e-20W.m**-2phot.flux;spect.line;em.line.Halphadoublenullablee_FnHa[11/6961]? Measurement error in FnHa1e-20W.m**-2stat.errorfloatnullableFWHMNII6549[353/1205]? FWHM of [NII]6549km/sspect.line.widthfloatnullablee_FWHMNII6549[0.4/348]? Measurement error in FWHMNII6549km/sstat.errorfloatnullableEWNII6549[2.7/1816]? Rest-frame equivalent width of [NII]65490.1nmspect.line.eqWidthdoublenullablee_EWNII6549[2.8/3583]? Measurement error in EWNII65490.1nmstat.errordoublenullableFNII6549[40/11937]? Flux of [NII]6549, 10-17erg/s/cm21e-20W.m**-2phot.fluxdoublenullablee_FNII6549[8/4359]? Measurement error in FNII65491e-20W.m**-2stat.errorfloatnullableFWHMNII6585[453/1205]? FWHM of [NII]6585km/sspect.line.widthfloatnullablee_FWHMNII6585[0.14/304]? Measurement error in FWHMNII6585km/sstat.errorfloatnullableEWNII6585[1.8/1038]? Rest-frame equivalent width of [NII]65850.1nmspect.line.eqWidthdoublenullablee_EWNII6585[4/570]? Measurement error in EWNII65850.1nmstat.errordoublenullableFNII6585[187/15319]? Flux of [NII]6585, 10^-17^erg/s/cm21e-20W.m**-2phot.fluxdoublenullablee_FNII6585[12/3455]? Measurement error in FNII65851e-20W.m**-2stat.errorfloatnullableFWHMSII6718[353/1204]? FWHM of [SII]km/sspect.line.widthfloatnullablee_FWHMSII6718[0.15/364]? Measurement error in FWHMSII6718km/sstat.errorfloatnullableEWSII6718[0.4/166]? Rest-frame equivalent width of [SII]MgII67180.1nmspect.line.eqWidthdoublenullablee_EWSII6718[1/57]? Measurement error in EWSII67180.1nmstat.errordoublenullableFSII6718[12/1282]? Flux of [SII]MgII6718, 10^-17^erg/s/cm21e-20W.m**-2phot.fluxfloatnullablee_FSII6718[5/440]? Measurement error in FSII67181e-20W.m**-2stat.errorfloatnullableFWHMSII6732[453/1205]? FWHM of [SII]MgII6732km/sspect.line.widthfloatnullablee_FWHMSII6732[0.14/330]? Measurement error in FWHMSII6732km/sstat.errorfloatnullableEWSII6732[0.29/55]? Rest-frame equivalent width of [SII]MgII67320.1nmspect.line.eqWidthdoublenullableMQsDisplay data from the million quasars cat. (VII/290) within 1"meta.ref.urlintnullablePapIDisplay data from Paper I (Fu+, 2021, J/ApJS/254/6)meta.ref.urlintnullableJ/ApJS/261/32/tablec1List of the stellar and galaxy contaminantsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameDesignation (JHHMMSS.ss+DDMMSS.s) (G1)meta.id;meta.maincharRAJ2000[2.3/300] PS1 right ascension (J2000) (G2)degpos.eq.ra;meta.mainDEJ2000[4.4/62.1] PS1 declination (J2000) (G2)degpos.eq.dec;meta.mainGLON[80.3/212.5] Galactic longitudedegpos.galactic.lonGLAT[-3.9/17] Galactic latitudedegpos.galactic.latdoubleClassClass ("star" or "galaxy")src.class.starGalaxycharimag[15.12/19.65] Mean PSF AB magnitude from PS1 i-filter detectionsmagphot.mag;em.opt.Ifloatz[0.04/0.11]? Redshift from visual inspectionsrc.redshiftfloatnullableMJD[58252.85/59229.3] Modified Julian Date of spectroscopic observation (JD-2400000.5)dtime.epochdoubleTelTelescopemeta.id;instr.telchar