J/A+A/691/A308/catalogCatalogNUV-r? Rest-frame NUV-r color (AB) (NUVR)magphot.color;em.UV;em.optdoublenullabler-K? Rest-frame r-K color (AB) (RK)magphot.color;em.IR;em.IRdoublenullableU-V? Rest-frame U-V color (AB) (UV)magphot.color;em.opt.U;em.opt.VdoublenullableV-J? Rest-frame V-J color (AB) (VJ)magphot.color;em.opt.V;em.IR.Jdoublenullableg-r? Rest-frame g-r color (AB) (GR)magphot.color;em.opt;em.optdoublenullablee_Lnu-u? Error of the rest-frame luminosity in a given band (LNU_U_ERR)W/Hzstat.errordoublenullablee_Lnu-g? Error of the rest-frame luminosity in g band (LNU_G_ERR)W/Hzstat.errordoublenullablee_Lnu-r? Error of the rest-frame luminosity in r band (LNU_R_ERR)W/Hzstat.errordoublenullablee_Lnu-i? Error of the rest-frame luminosity in i band (LNU_I_ERR)W/Hzstat.errordoublenullablee_Lnu-z? Error of the rest-frame luminosity in z band (LNU_Z_ERR)W/Hzstat.errordoublenullablee_NUV-r? Error of the rest-framed color NUV-r (NUVR_ERR)magstat.errordoublenullablee_r-K? Error of the rest-framed color r-K (RK_ERR)magstat.errordoublenullablee_U-V? Error of the rest-framed color U-V (UV_ERR)magstat.error;phot.color;em.opt.Udoublenullablee_V-J? Error of the rest-framed color V-J (VJ_ERR)magstat.error;phot.color;em.opt.Vdoublenullablee_g-r? Error of the rest-framed color g-r (GR_ERR)magstat.error;phot.color;em.opt.BdoublenullableFlag-MassPDFFlag expressed by Mbest/Mbayes to reject stellar mass estimates with broad PDF and/or complex likelihood distribution (FLAG_MASSPDF) (3)meta.code.errordoubleFlag-SFRPDFFlag expressed by SFRbest/SFRbayes to reject SFR estimates with broad PDF and/or complex likelihood distribution (FLAG_SFRPDF) (4)meta.code.errordoubleFlag-OptFlag to preselect sources observed with high signal-to-noise (S/N>=10 in optical bands(g, r, z) (FLAGOPTICAL) (5)meta.code.errorintFlag-IRFlag to preselect sources observed with high signal-to-noise (S/N>=3 in WISE bands(W1, W2, W3, W4) (FLAGINFRARED) (6)meta.code.errorintFluxgFlux in g band in nanomaggy (FLUX_G) (7)3.63uJyphot.mag;em.opt.BdoubleFluxrFlux in r band in nanomaggy (FLUX_R) (7)3.63uJyphot.mag;em.opt.RdoubleFluxzFlux in z band in nanomaggy (FLUX_Z) (7)3.63uJyphot.mag;em.opt.IdoubleFluxW1Flux in W1 band in nanomaggy (FLUX_W1) (7)3.63uJyphot.mag;em.IR.3-4umdoubleFluxW2Flux in W2 band in nanomaggy (FLUX_W2) (7)3.63uJyphot.mag;em.IR.4-8umdoubleFluxW3Flux in W3 band in nanomaggy (FLUX_W3) (7)3.63uJyphot.flux.density;em.IR.8-15umdoubleFluxW4Flux in W4 band in nanomaggy (FLUX_W4) (7)3.63uJyphot.flux.density;em.IR.15-30umdoubleSNR-gSignal-to-noise in g band calculated as FLUX*sqrt(FLUX_IVAR) (SNR_G)stat.snrdoubleFlux-ivargInverse variance of the flux in g band in nanomaggy^-2^ (FLUX_IVAR_G)3.63uJy**-2phot.mag;em.opt.BdoubleFlux-ivarrInverse variance of the flux in r band in nanomaggy^-2^ (FLUX_IVAR/R)3.63uJy**-2phot.mag;em.opt.RdoubleFlux-ivarzInverse variance of the flux in z band in nanomaggy^-2^ (FLUX_IVAR_Z)3.63uJy**-2phot.mag;em.opt.IdoubleFlux-ivarW1Inverse variance of the flux in W1 band in nanomaggy^-2^ (FLUX_IVAR_W1)3.63uJy**-2phot.mag;em.IR.3-4umdoubleFlux-ivarW2Inverse variance of the flux in W2 band in nanomaggy^-2^ (FLUX_IVAR_W2)3.63uJy**-2phot.mag;em.IR.4-8umdoubleFlux-ivarW3Inverse variance of the flux in W3 band in nanomaggy^-2^ (FLUX_IVAR_W3)3.63uJy**-2phot.flux.density;em.IR.8-15umdoubleFlux-ivarW4Inverse variance of the flux in W4 band in nanomaggy^-2^ (FLUX_IVAR_W4)3.63uJy**-2phot.flux.density;em.IR.15-30umdoubleMWTransg[0/1] Milky Way foreground dust transmission factor in g band (MW_TRANSMISSION_G)instr.paramdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTargetUnique DESI Target ID (TARGETID)meta.id;meta.mainSurveySurvey name (SURVEY)meta.idcharHEALPIXHealpix number (HEALPIX)meta.numberintRAJ2000Right ascension (J2000) from target catalog (RA)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) from target catalog (DEC)degpos.eq.dec;meta.mainindexedReleaseLegacy Surveys (LS) Release (RELEASE)meta.softwareintzRedshift (Z)src.redshiftdoublechi2? Reduced chi2 defining the quality of the fit: for a more reliable estimations the cut of chi2<~15 is recommended (CHI2)stat.fit.chi2;stat.fit.param;meta.modelledfloatnullablelogM? logarithm of the stellar mass (LOGM)log(solMass)phys.massdoublenullablee_logM? Error on logarithm of the stellar mass (LOGM_ERR)log(solMass)stat.errordoublenullablelogSFR? logarithm of the star formation rate averaged over 10Myr (LOGSFR)log(solMass.yr**-1)phys.SFRdoublenullablee_logSFR? Error on logarithm of star formation rate averaged over 10Myr (LOGSFR_ERR)log(solMass.yr**-1)stat.error;phys.SFRdoublenullableAGNLumTotal Luminosity of the AGN (AGNLUM)Wphys.luminositydoubleAGNFrac? Fraction of the total IR emission coming from the AGN (AGNFRAC) (1)phys.luminosity;arith.ratiodoublenullableAGNPsy? Viewing angle, with ~30deg and ~70deg, for type 1 and type 2 AGN, respectively (AGNPSY)degpos.posAngdoublenullableLnu-uRest-frame luminosity in u band (LNU_U) (2)W/Hzphys.luminositydoubleLnu-gRest-frame luminosity in g band (LNU_G) (2)W/Hzphys.luminositydoubleLnu-rRest-frame luminosity in r band (LNU_R) (2)W/Hzphys.luminositydoubleLnu-iRest-frame luminosity in i band (LNU_I) (2)W/Hzphys.luminositydoubleLnu-zRest-frame luminosity in z band (LNU_Z) (2)W/Hzphys.luminositydoubleMWTransr[0/1] Milky Way foreground dust transmission factor in r band (MW_TRANSMISSION_R)instr.paramdoubleMWTransz[0/1] Milky Way foreground dust transmission factor in z band (MW_TRANSMISSION_Z)instr.paramdoubleMWTransW1[0/1] Milky Way foreground dust transmission factor in W1 band (MW_TRANSMISSION_W1)instr.paramdoubleMWTransW2[0/1] Milky Way foreground dust transmission factor in W2 band (MW_TRANSMISSION_W2)instr.paramdoubleMWTransW3[0/1] Milky Way foreground dust transmission factor in W3 band (MW_TRANSMISSION_W3)instr.paramdoubleMWTransW4[0/1] Milky Way foreground dust transmission factor in W3 band (MW_TRANSMISSION_W4)instr.paramdoubleSNR-rSignal-to-noise in r band calculated as FLUX*sqrt(FLUX_IVAR) (SNR_R)stat.snrdoubleSNR-zSignal-to-noise in z band calculated as FLUX*sqrt(FLUX_IVAR) (SNR_Z)stat.snrdoubleSNR-W1Signal-to-noise in W1 band calculated as FLUX*sqrt(FLUX_IVAR) (SNR_W1)stat.snrdoubleSNR-W2Signal-to-noise in W2 band calculated as FLUX*sqrt(FLUX_IVAR) (SNR_W2)stat.snrdoubleSNR-W3Signal-to-noise in W3 band calculated as FLUX*sqrt(FLUX_IVAR) (SNR_W3)stat.snrdoubleSNR-W4Signal-to-noise in W4 band calculated as FLUX*sqrt(FLUX_IVAR) (SNR_W4)stat.snrdoubleProgramProgram name (PROGRAM)meta.id;obscharSpTypeRedrock spectral classification (SPECTYPE)src.spTypechar