J/ApJ/922/179/table2cThe WISE AGN galaxy catalog; from erratum published in 2023, ApJ, 952, 171recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/695273] Catalog specific unique IDmeta.idintRAJ2000WISE source right ascension (J2000)degpos.eq.ra;meta.mainindexedDEJ2000[-30/89.6] WISE source declination (J2000)degpos.eq.dec;meta.mainindexedzspec[-0.009/7.02]? SDSS DR16 spectroscopic redshift (1)src.redshiftdoublenullablezphot[0.01/4] Photometric redshiftsrc.redshiftfloatzbest[0.0001/7.02] Best redshiftsrc.redshiftfloatn_zbestBest redshift type "spec" or "phot"meta.notecharLbolagn[6.7e+36/3.4e+49] AGN component bolometric luminosity1e-07Wphys.luminositydoubleb_Lbolagn[6.2e+36/3.2e+49] The 16th percentile uncertainty in Lbolagn1e-07Wstat.errordoubleB_Lbolagn[7.2e+36/3.6e+49] The 84th percentile uncertainty in Lbolagn1e-07Wstat.errordoubleEBV[0/4.5] AGN color excessmagphot.color.excessfloatb_EBV[0/3.3] The 16th percentile uncertainty in EBVmagstat.error;phot.magfloatB_EBV[0.005/5.6] The 84th percentile uncertainty in EBVmagstat.error;phot.magfloatMstar[1e+7/4e+15]? Host galaxy stellar mass (1)solMassphys.massdoublenullableb_Mstar[2846/4e+15]? The 16th percentile uncertainty in MstarsolMassstat.errordoublenullableB_Mstar[1e+7/4.1e+15]? The 84th percentile uncertainty in MstarsolMassstat.errordoublenullableSFR[0/2.1e+6]? Host galaxy star formation rate (1)solMass/yrphys.SFRdoublenullableb_SFR[0/854100]? The 16th percentile uncertainty in SFRsolMass/yrstat.error;phys.SFRdoublenullableB_SFR[0.01/3.4e+6]? The 84th percentile uncertainty in SFRsolMass/yrstat.error;phys.SFRdoublenullableL2800[2e+35/1.1e+48] 2800 monochromatic AGN luminosity1e-07Wphys.luminositydoubleb_L2800[2e+35/1.1e+48] The 16th percentile uncertainty in L28001e-07Wstat.errordoubleB_L2800[2.3e+35/1.2e+48] The 84th percentile uncertainty in L28001e-07Wstat.errordoubleLE[8.6e+35/6.3e+48]? Elliptical component bolometric luminosity1e-07Wphys.luminositydoublenullableb_LE[5.7e+35/5.5e+48]? The 16th percentile uncertainty in LSbc1e-07Wstat.errordoublenullableB_LE[1e+36/7e+48]? The 84th percentile uncertainty in LSbc1e-07Wstat.errordoublenullableLSbc[1.5e+35/8.5e+48]? Spiral component bolometric luminosity1e-07Wphys.luminositydoublenullableb_LSbc[9e+34/6.6e+48]? The 16th percentile uncertainty in LSbc1e-07Wstat.errordoublenullablee_iobs[2.7e-7/1.4e-5]? Uncertainty in iobsJystat.errordoublenullablee_Grpobs[8e-9/0.002]? Uncertainty in GrpobsJystat.errordoublenullableB_LSbc[2e+35/1.1e+49]? The 84th percentile uncertainty in LSbc1e-07Wstat.errordoublenullableLIm[8.2e+35/2.8e+48]? Irregular component bolometric luminosity1e-07Wphys.luminositydoublenullableb_LIm[6e+35/2.1e+48]? The 16th percentile uncertainty in LIm1e-07Wstat.errordoublenullableB_LIm[1e+36/3.5e+48]? The 84th percentile uncertainty in LIm1e-07Wstat.errordoublenullableFUVmod[1e-36/0.002]? GALEX FUV band model flux density (few values <1e-37 have been set to 0 by CDS)Jyphot.flux;meta.modelleddoublenullableNUVmod[2.5e-22/0.002] GALEX NUV band model flux densityJyphot.flux;meta.modelleddoubleumod[1.3e-17/0.003] SDSS DR14 u band model flux densityJyphot.flux;meta.modelleddoublegmod[3e-17/0.004] SDSS DR14 or Pan-STARRS DR2 g band model flux densityJyphot.flux;meta.modelleddoubleGbpmod[1.4e-7/0.004] Gaia DR2 blue passband model flux densityJyphot.flux;meta.modelleddoublermod[4.7e-7/0.005] SDSS DR14 or Pan-STARRS DR2 r band model flux densityJyphot.flux;meta.modelleddoubleimod[1.9e-6/0.005] SDSS DR14 or Pan-STARRS DR2 i band model flux densityJyphot.flux;meta.modelleddoubleGrpmod[2e-6/0.005] Gaia DR2 red passband model flux densityJyphot.flux;meta.modelleddoublezmod[2.4e-6/0.006] SDSS DR14 or Pan-STARRS DR2 z band model flux densityJyphot.flux;meta.modelleddoubleymod[2.6e-6/0.007] Pan-STARRS DR2 y band flux densityJyphot.flux;meta.modelleddoubleJmod[2.8e-6/0.009] 2MASS PSC J band model flux densityJyphot.flux;meta.modelleddoubleHmod[2.7e-6/0.02] 2MASS PSC H band model flux densityJyphot.flux;meta.modelleddoubleKsmod[4.5e-6/0.02] 2MASS PSC Ks band model flux densityJyphot.flux;meta.modelleddoubleW1mod[1e-5/0.04] WISE W1 band, 3.4um, model flux densityJyphot.flux;meta.modelleddoubleW2mod[1.7e-5/0.07] WISE W2 band, 4.6um, model flux densityJyphot.flux;meta.modelleddoubleW3mod[4.2e-5/0.3] WISE W3 band, 12.1um, model flux densityJyphot.flux;meta.modelleddoubleW4mod[9.5e-5/0.5] WISE W4 band, 22.2um, model flux densityJyphot.flux;meta.modelleddoubleFUVkcor[2e-36/5.1]? GALEX FUV band photometric k-correction (few values <1e-37 have been set to 0 by CDS)arith.factor;phot.magdoublenullableNUVkcor[2e-17/6.6] GALEX NUV band photometric k-correctionarith.factor;phot.magdoubleukcor[3.9e-13/7.5] SDSS DR14 u band photometric k-correctionarith.factor;phot.magdoublegkcor[6.7e-13/5] SDSS DR14 or Pan-STARRS DR2 g band photometric k-correctionarith.factor;phot.magdoubleGbpkcor[0.006/4.7] Gaia DR2 blue passband photometric k-correctionarith.factor;phot.magdoublerkcor[0.01/5] SDSS DR14 or Pan-STARRS DR2 r band photometric k-correctionarith.factor;phot.magdoubleikcor[0.01/5.8] SDSS DR14 or Pan-STARRS DR2 i band photometric k-correctionarith.factor;phot.magdoubleGrpkcor[0.01/5.2] Gaia DR2 red passband photometric k-correctionarith.factor;phot.magdoublezkcor[0.02/5.5] SDSS DR14 or Pan-STARRS DR2 z band photometric k-correctionarith.factor;phot.magdoubleykcor[0.02/5.6] Pan-STARRS DR2 y band flux densityarith.factor;phot.magdoubleJkcor[0.02/4.1] 2MASS PSC J band photometric k-correctionarith.factor;phot.magdoubleHkcor[0.04/2.9] 2MASS PSC H band photometric k-correctionarith.factor;phot.magdoubleKskcor[0.04/4.3] 2MASS PSC Ks band photometric k-correctionarith.factor;phot.magdoubleW1kcor[0.03/9.2] WISE W1 band, 3.4um, photometric k-correctionarith.factor;phot.magdoubleW2kcor[0.05/15.2] WISE W2 band, 4.6um, photometric k-correctionarith.factor;phot.magdoubleW3kcor[0.2/30] WISE W3 band, 12.1um, photometric k-correctionarith.factor;phot.magdoubleW4kcor[0.3/8] WISE W4 band, 22.2um, photometric k-correctionarith.factor;phot.magdoubleFUVobs[1.1e-7/0.09]? GALEX FUV band observed flux density (1)Jyphot.flux;em.UVdoublenullablee_FUVobs[3e-8/0.0006]? Uncertainty in FUVobsJystat.errordoublenullableNUVobs[2.4e-8/0.05]? GALEX NUV band observed flux density (1)Jyphot.flux;em.UVdoublenullablee_NUVobs[4.8e-8/0.0002]? Uncertainty in NUVobsJystat.errordoublenullableuobs[1e-10/0.05]? SDSS DR14 u band observed flux density (1)Jyphot.flux.density;em.opt.Udoublenullablee_uobs[4.7e-13/152]? Uncertainty in uobsJystat.errordoublenullablegobs[5.6e-9/0.004]? SDSS DR14 or Pan-STARRS DR2 g band observed flux density (1)Jyphot.flux.density;em.opt.Bdoublenullablee_gobs[1.6e-7/2e-5]? Uncertainty in gobsJystat.errordoublenullableGbpobs[3.5e-7/0.1]? Gaia DR2 blue passband observed flux density (1)Jyphot.flux.density;em.opt.Bdoublenullablee_Gbpobs[7.3e-10/0.002]? Uncertainty in GbpobsJystat.errordoublenullablerobs[1.5e-7/0.005]? SDSS DR14 or Pan-STARRS DR2 r band observed flux density (1)Jyphot.flux.density;em.opt.Rdoublenullablee_robs[1.8e-7/3.1e-5]? Uncertainty in robsJystat.errordoublenullableiobs[3.8e-7/0.006]? SDSS DR14 or Pan-STARRS DR2 i band observed flux density (1)Jyphot.flux.density;em.opt.IdoublenullableGrpobs[2.4e-6/0.2]? Gaia DR2 red passband observed flux density (1)Jyphot.flux.density;em.opt.Rdoublenullablezobs[6.5e-7/0.006]? SDSS DR14 or Pan-STARRS DR2 z band observed flux density (1)Jyphot.flux.density;em.opt.Idoublenullablee_zobs[5.9e-7/3.4e-5]? Uncertainty in zobsJystat.errordoublenullableyobs[4.2e-7/0.007]? Pan-STARRS DR2 y band flux density (1)Jyphot.mag;em.IR.Jdoublenullablee_yobs[1.3e-6/8e-5]? Uncertainty in yobsJystat.errordoublenullableJobs[3e-5/0.2]? 2MASS PSC J band observed flux density (1)Jyphot.flux.density;em.IR.Jdoublenullablee_Jobs[3e-6/0.005]? Uncertainty in JobsJystat.errordoublenullableHobs[5.4e-5/0.2]? 2MASS PSC H band observed flux density (1)Jyphot.flux.density;em.IR.Hdoublenullablee_Hobs[5.4e-6/0.004]? Uncertainty in HobsJystat.errordoublenullableKsobs[6.2e-5/0.09]? 2MASS PSC Ks band observed flux density (1)Jyphot.mag;em.IR.Kdoublenullablee_Ksobs[6.2e-6/0.003]? Uncertainty in KsobsJystat.errordoublenullableW1obs[9.4e-6/0.04] WISE W1 band, 3.4 um, observed flux densityJyphot.mag;em.IR.3-4umdoublee_W1obs[2e-6/0.001]? Uncertainty in W1Jystat.errordoublenullableW2obs[3.8e-5/0.07] WISE W2 band, 4.6 um, observed flux densityJyphot.mag;em.IR.4-8umdoublee_W2obs[4.2e-6/0.002]? Uncertainty in W2Jystat.errordoublenullableW3obs[9.9e-5/0.2]? WISE W3 band, 12.1 um, observed flux density (1)Jyphot.flux.density;em.IR.8-15umdoublenullablee_W3obs[4e-5/0.003]? Uncertainty in W3Jystat.errordoublenullableW4obs[0.0006/0.5]? WISE W4 band, 22.2 um, observed flux density (1)Jyphot.flux.density;em.IR.15-30umdoublenullablee_W4obs[0.0003/0.03]? Uncertainty in W4Jystat.errordoublenullableWISEAWISE source name (JHHMMSS.ss+DDMMSS.s)meta.id;meta.mainchar