J/A+A/702/A187ivo://CDS.VizieR/J/A+A/702/A187doi:10.26093/cds/vizier/bc-ny/lbihCDSDe Daniloff S.B.Bongiovanni A.Sanchez-Portal M.Cedres B.,Padilla-Torres C.P.Perez-Garcia A.M.Perez-Martinez R.Espada D.,de la Casa C.C.Torres-Rios G.Gonzalez-Otero M.de Diego J.A.,Rodriguez M.I.Cervino M.Lara-Lopez M.A.Cepa J.Valtchanov I.,Gonzalez-Serrano J.I.Cruz-Gonzalez I.Negrete C.A.Beyoro-Amado Z.,Castillo-Fraile M.Mancillas B.Povic M.2026-08-03T06:58:00Z2025-11-23T10:18:15ZCDS support team

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

cds-question@unistra.frgalaxiesvisible-astronomycatalogsspectroscopyphotometrystellar-evolutionary-modelsGalaxy clusters are among the largest and densest structures in the Universe. Their high density generally increases the suppression of star formation, known as quenching, altering galaxy properties. We study the quenching of emission-line galaxies (ELGs) in the rich cluster ZwCl 0024.0+1652 (Cl0024) at redshift z~0.4, aiming to determine if and how star formation is suppressed. Using multi-object spectroscopy from the GLACE survey, we extract fluxes and redshifts of [OII]3727,3729, Hbeta}, and [OIII]5007 emission lines to derive star formation rates (SFRs) for 173 ELGs. We also perform spectral energy distribution fitting to obtain key evolutionary parameters such as stellar masses and the 4000 Angstrom break (D4000) index. We derive the stellar mass-SFR relation for 98 star-forming galaxies, finding 34.7% exhibit suppressed SFRs in the cluster, compared to 11.0% in the field. While SFRs show no significant variation with local density, the fraction of SFGs is 1.55 times higher in the cluster outskirts than in intermediate-density regions. The specific SFR decreases strongly with $D4000$ for active SFGs but remains constant for suppressed galaxies. The fraction of suppressed galaxies in the infall region is 2.6 times higher than in the core, and especially in the infalling structure B of the cluster. The cluster's total mass does not appear to be a key factor in SFG quenching. Star formation in Cl0024 galaxies is suppressed by the dense cluster environment. This suppression is evident in SFG fractions and parameters tracing long-term evolution, indicating prolonged quenching. SFGs preferentially reside in low-density regions, while suppressed galaxies dominate the infall region, supporting a "delayed-then-rapid" quenching scenario.2025A&A...702A.187Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/702/A187CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/501/2430 : Galaxy activity in ZwCl0024+1652 clusterhttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/702/A187https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/702/A187http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/702/A187https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/702/A187https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/702/A187http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/702/A187GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/702/A187/catalog (Catalog of the properties of the galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/702/A187/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/702/A187/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/702/A187/catalog?GETtext/xml+votable180.050000true6.642771517.10123650.0055555555555555566/198467.952274030004205e-20 5.125927419590277e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/702/A187?format=asciiOpticaldefaultJ/A+A/702/A187/catalogCatalog of the properties of the galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-uniqueGLACE ID with pointing label, NNNNN_a (id_unique) (1)(2)meta.id;meta.maincharIDGLACE ID without pointing label (ID) (1)meta.idinte_FHaSP15Error in flux of Halpha emission line (e_F_Halpha_SP15) (1)mW.m**-2stat.errordoubleFNIISP15? Flux of [NII]6548 emission line (F_NII_SP15) (1)mW.m**-2phot.flux;spect.linedoublenullableFOII? Flux of [OII] emission line (F_OII)mW.m**-2phot.flux;spect.linedoublenullablelogM*? Logarithm of the stellar mass obtained from CSP (logStellar_mass)log(solMass)phys.massdoublenullablee_logM*? Error in logarithm of the stellar mass obtained from CSP (e_logStellar_mass)log(solMass)stat.errordoublenullableisAGNWHAN[0/1]? True/False flag for AGN activity based on EWalphaN2 (Ho+1997); NaN if not conclusive (isAGN_WHAN)meta.codefloatnullableID-MOSID of the MOS spectrum after reduction (id_MOS)meta.idcharRAJ2000Right ascension (J2000) from TF (tunable filters) calibrated data (RA_J2000) (1)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) from TF calibrated data (DEC_J2000) (1)degpos.eq.dec;meta.mainRAGdegRight ascension from GAIA-DR1 (ICRS) at Ep=2015.0 (RA_GAIA) (1)degpos.eq.raDEGdegDeclination from GAIA- DR1 (ICRS) at Ep=2015.0 (DEC_GAIA) (1)degpos.eq.deczSP15Redshift from TF calibrated data (Sanchez-Portal et al., 2015A&A...578A..30S,) (z_SP15)src.redshift;pos.heliocentricdoublezHaICRedshift of Halpha emission line obtained from inverse convolution method (z_Halpha_InvConv) (3)src.redshift;pos.heliocentricdoubleb_zHaICLower value of redshift of Halpha emission line (z_Halpha_InvConv_d) (3)src.redshift;stat.mindoubleB_zHaICUpper value of redshift of Halpha emission line (z_Halpha_InvConv_u) (3)src.redshift;stat.maxdoublezOII? Redshift of [OII] emission line (z_OII)src.redshift;pos.heliocentricdoublenullablee_zOII? Error in redshift of [OII] emission line (e_z_OII)stat.errordoublenullablezHb? Redshift of Hbeta emission line (z_Hbeta)src.redshift;pos.heliocentricdoublenullablee_zHb? Error in redshift of Hbeta emission line (e_z_Hbeta)stat.errordoublenullablezOIII? Redshift of [OIII]5007 emission line (z_OIII)src.redshift;pos.heliocentricdoublenullablee_zOIII? Error in redshift of [OIII]5007 emission line (e_z_OIII)stat.errordoublenullablezMOSavg? Average redshift of [OII], Hbeta, and [OIII]5007 emission lines (z_MOS_avg)src.redshift;pos.heliocentricdoublenullablee_zMOSavg? Error in average redshift of [OII], Hbeta, and [OIII]5007 emission lines (e_z_MOS_avg)stat.errordoublenullableBmag? B-band (CFHT/CFH12k) AUTO magnitude (Vega system); automatic aperture from SExtractor; proxy for total magnitude (B_AUTO) (1)magphot.mag;em.opt.Bdoublenullablee_Bmag? Error in B-band AUTO magnitude (e_B_AUTO) (1)magstat.error;phot.magdoublenullableVmag? V-band (CFHT/CFH12k) AUTO magnitude V_AUTO) (1)magphot.mag;em.opt.Vdoublenullablee_Vmag? Error in V-band AUTO magnitude (e_V_AUTO) (1)magstat.error;phot.magdoublenullableRmag? R-band (CFHT/CFH12k) AUTO magnitude (R_AUTO) (1)magphot.mag;em.opt.Rdoublenullablee_Rmag? Error in R-band AUTO magnitude (e_R_AUTO) (1)magstat.error;phot.magdoublenullableImag? I-band (CFHT/CFH12k) AUTO magnitude (I_AUTO) (1)magphot.mag;em.opt.Idoublenullablee_Imag? Error in I-band AUTO magnitude (e_I_AUTO) (1)magstat.error;phot.magdoublenullableJmag? J-band (Palomar200/WIRC) AUTO magnitude (J_AUTO) (1)magphot.mag;em.IR.Jdoublenullablee_Jmag? Error in J-band AUTO magnitude (e_J_AUTO) (1)magstat.error;phot.magdoublenullableKsmag? Ks-band (Palomar200/WIRC) AUTO magnitude (Ks_AUTO) (1)magphot.mag;em.IR.Kdoublenullablee_Ksmag? Error in Ks-band AUTO magnitude (e_Ks_AUTO) (1)magstat.error;phot.magdoublenullableF814Wmag? HST/WFPC2 814nm wide band AUTO magnitude (F814W_AUTO) (1)magphot.mag;em.opt.Idoublenullablee_F814Wmag? Error in HST/WFPC2 814nm wide band AUTO magnitude (e_F814W_AUTO) (1)magstat.errordoublenullableFHaSP15Flux of Halpha emission line (F_Halpha_SP15) (1)mW.m**-2phot.flux;em.line.Halphadoublee_FNIISP15? Error in flux of [NII]6548 emission line (e_FNII_SP15) (1)mW.m**-2stat.errordoublenullableFHacSP15Flux of Halpha adjusted and corrected for absorptions and extinction (FHalpha_corrected_SP15) (1)mW.m**-2phot.flux;em.line.Halphadoublee_FHacSP15Error in flux of Halpha adjusted and corrected for absorptions and extinction (eFHalpha_corrected_SP15) (1)mW.m**-2stat.errordoubleFNIIcSP15? Flux of [NII]6548 adjusted and corrected for absorptions and extinction (FNII_corrected_SP15) (1)mW.m**-2phot.fluxdoublenullablee_FNIIcSP15? Error in flux of [NII]6548 adjusted and corrected for absorptions and extinction (eFNII_corrected_SP15) (1)mW.m**-2stat.errordoublenullableEWHaSP15Equivalent width of Halpha emission line obtained from tunable filters (EW_Halpha_SP15) (1)0.1nmspect.line.eqWidthdoublee_EWHaSP15Error in equivalent width of Halpha emission line obtained from tunable filters (e_EW_Halpha_SP15) (1)0.1nmstat.errordoubleContHaICContinuum level of Halpha line obtained from inverse convolution (Cont_Halpha_InvConv) (3)10mW.m**-2.nm**-1phot.flux;em.line.Halphadoubleb_ContHaICLower value of continuum level of Halpha line obtained from inverse convolution (Cont_Halpha_InvConv_d) (3)10mW.m**-2.nm**-1stat.stdev;stat.mindoubleB_ContHaICUpper value of continuum level of Halpha line obtained from inverse convolution (Cont_Halpha_InvConv_u) (3)10mW.m**-2.nm**-1stat.stdev;stat.maxdoublesigmaHaICSigma of the Gaussian fit for Halpha line obtained from inverse convolution (sigma_Halpha_InvConv) (3)0.1nmstat.fit.param;meta.modelleddoubleb_sigmaHaICLower value of sigma of the Gaussian fit for Halpha line obtained from inverse convolution (sigma_Halpha_InvConv_d) (3)0.1nmstat.stdev;stat.mindoubleB_sigmaHaICUpper value of sigma of the Gaussian fit for Halpha line obtained from inverse convolution (sigma_Halpha_InvConv_u) (3)0.1nmstat.stdev;stat.maxdoubleFNII6548ICFlux of [NII]6548 emission line obtained from inverse convolution (F_NII6548_InvConv) (3)mW.m**-2phot.flux;spect.linedoubleb_FNII6548ICLower value of flux of [NII]6548 emission line obtained from inverse convolution (F_NII6548_InvConv_d) (3)mW.m**-2phot.flux;stat.mindoubleB_FNII6548ICUpper value of flux of [NII]6548 emission line obtained from inverse convolution (F_NII6548_InvConv_u) (3)mW.m**-2phot.flux;stat.maxdoubleFHaICFlux of Halpha emission line obtained from inverse convolution (F_Halpha_InvConv) (3)mW.m**-2phot.flux;em.line.Halphadoubleb_FHaICLower value of flux of Halpha obtained from inverse convolution (F_Halpha_InvConv_d) (3)mW.m**-2phot.flux;stat.mindoubleB_FHaICUpper value of flux of Halpha obtained from inverse convolution (F_Halpha_InvConv_u) (3)mW.m**-2phot.flux;stat.maxdoubleFNII6583ICFlux of [NII]6583 emission line obtained from inverse convolution (F_NII6583_InvConv) (3)mW.m**-2phot.flux;spect.linedoubleb_FNII6583ICLower value of flux of [NII]6583 obtained from inverse convolution (F_NII6583_InvConv_d) (3)mW.m**-2phot.flux;stat.mindoubleB_FNII6583ICUpper value of flux of [NII]6583 obtained from inverse convolution (F_NII6583_InvConv_u) (3)mW.m**-2phot.flux;stat.maxdoubleEWNII6548ICEquivalent width of [NII]6548 emission line obtained from inverse convolution (EW_NII6548_InvConv) (3)0.1nmspect.line.eqWidthdoubleb_EWNII6548ICLower value of equivalent width of [NII]6548 emission line obtained from inverse convolution (EW_NII6548_InvConv_d) (3)0.1nmspect.line.eqWidth;stat.mindoubleB_EWNII6548ICUpper value of equivalent width of [NII]6548 emission line obtained from inverse convolution (EW_NII6548_InvConv_u) (3)0.1nmspect.line.eqWidth;stat.maxdoubleEWHaICEquivalent width of Halpha emission line obtained from inverse convolution (EW_Halpha_InvConv) (3)0.1nmspect.line.eqWidthdoubleb_EWHaICLower value of equivalent width of Halpha emission line obtained from inverse convolution (EW_Halpha_InvConv_d) (3)0.1nmspect.line.eqWidth;stat.mindoubleB_EWHaICUpper value of equivalent width of Halpha emission line obtained from inverse convolution (EW_Halpha_InvConv_u) (3)0.1nmspect.line.eqWidth;stat.maxdoubleEWNII6583ICEquivalent width of [NII]6583 emission line obtained from inverse convolution (EW_NII6583_InvConv) (3)0.1nmspect.line.eqWidthdoubleb_EWNII6583ICLower value of equivalent width of [NII]6583 emission line obtained from inverse convolution (EW_NII6583_InvConv_d) (3)0.1nmspect.line.eqWidth;stat.mindoubleB_EWNII6583ICUpper value of equivalent width of [NII]6583 emission line obtained from inverse convolution (EW_NII6583_InvConv_u) (3)0.1nmspect.line.eqWidth;stat.maxdoubleEWOII? Equivalent width of [OII] emission line (EW_OII)0.1nmspect.line.eqWidthdoublenullablee_EWOII? Error in equivalent width of [OII] emission line (e_EW_OII)0.1nmstat.errordoublenullableEWHb? Equivalent width of Hbeta emission line (EW_Hbeta)0.1nmspect.line.eqWidthdoublenullablee_EWHb? Error in equivalent width of Hbeta emission line (e_EW_Hbeta)0.1nmstat.errordoublenullableEWOIII? Equivalent width of [OIII]5007 emission line (EW_OIII)0.1nmspect.line.eqWidthdoublenullablee_EWOIII? Error in equivalent width of [OIII]5007 emission line (e_EW_OIII)0.1nmstat.errordoublenullablecontOII? Continuum level of [OII] emission line (cont_OII)10mW.m**-2.nm**-1phot.fluxdoublenullablee_contOII? Error in continuum level of [OII] emission line (e_cont_OII)10mW.m**-2.nm**-1stat.errordoublenullablecontHb? Continuum level of Hbeta emission line (cont_Hbeta)10mW.m**-2.nm**-1phot.fluxdoublenullablee_contHb? Error in continuum level of Hbeta emission line (e_cont_Hbeta)10mW.m**-2.nm**-1stat.errordoublenullablecontOIII? Continuum level of [OIII]5007 emission line (cont_OIII)10mW.m**-2.nm**-1phot.fluxdoublenullablee_contOIII? Error in continuum level of [OIII]5007 emission line (e_cont_OIII)10mW.m**-2.nm**-1stat.errordoublenullablecoreOII? Core (amplitude) of [OII] emission line (core_OII)10mW.m**-2.nm**-1phot.fluxdoublenullablee_coreOII? Error in core (amplitude) of [OII] emission line (e_core_OII)10mW.m**-2.nm**-1stat.errordoublenullablecoreHb? Core (amplitude) of Hbeta emission line (core_Hbeta)10mW.m**-2.nm**-1phot.flux;em.line.Hbetadoublenullablee_coreHb? Error in core (amplitude) of Hbeta emission line (e_core_Hbeta)10mW.m**-2.nm**-1stat.errordoublenullablecoreOIII? Core (amplitude) of [OIII]5007 emission line (core_OIII)10mW.m**-2.nm**-1phot.fluxdoublenullablee_coreOIII? Error in core (amplitude) of [OIII]5007 emission line (e_core_OIII)10mW.m**-2.nm**-1stat.errordoublenullablesigmaOII? sigma of the Gaussian fit for [OII] emission line (sigma_OII)0.1nmstat.fit.param;meta.modelleddoublenullablee_sigmaOII? Error in sigma of the Gaussian fit for [OII] emission line (e_sigma_OII)0.1nmstat.errordoublenullablesigmaHb? sigma of the Gaussian fit for Hbeta emission line (sigma_Hbeta)0.1nmstat.fit.param;meta.modelleddoublenullablee_sigmaHb? Error in sigma of the Gaussian fit for Hbeta emission line (e_sigma_Hbeta)0.1nmstat.errordoublenullablesigmaOIII? sigma of the Gaussian fit for [OIII]5007 emission line (sigma_OIII)0.1nmstat.fit.param;meta.modelleddoublenullablee_sigmaOIII? Error in sigma of the Gaussian fit for [OIII]5007 emission line (e_sigma_OIII)0.1nmstat.errordoublenullableFWHMOII? Full-Width at Half Maximum (FWHM) of the Gaussian fit for [OII] emission line (FWHM_OII)0.1nmspect.line.widthdoublenullablee_FWHMOII? Error in FWHM of the Gaussian fit for [OII] emission line (e_FWHM_OII)0.1nmstat.errordoublenullableFWHMHb? Full-Width at Half Maximum (FWHM) of the Gaussian fit for Hbeta emission line (FWHM_Hbeta)0.1nmspect.line.widthdoublenullablee_FWHMHb? Error in FWHM of the Gaussian fit for Hbeta emission line (e_FWHM_Hbeta)0.1nmstat.errordoublenullableFWHMOIII? Full-Width at Half Maximum (FWHM) of the Gaussian fit for [OIII]5007 emission line (FWHM_OIII)0.1nmspect.line.widthdoublenullablee_FWHMOIII? Error in FWHM of the Gaussian fit for [OIII]5007 emission line (e_FWHM_OIII)0.1nmstat.errordoublenullableSNRlineOII? Signal-to-Noise Ratio (S/N) of the [OII] emission line (SNR_line_OII)stat.snrdoublenullableSNRlineHb? Signal-to-Noise Ratio (S/N) of the Hbeta emission line (SNR_line_Hbeta)stat.snrdoublenullableSNRlineOIII? Signal-to-Noise Ratio (S/N) of the [OIII]5007 emission line (SNR_line_OIII)stat.snrdoublenullablee_FOII? Error in flux of [OII] emission line (e_F_OII)mW.m**-2stat.errordoublenullableFHb? Flux of Hbeta emission line (F_Hbeta)mW.m**-2phot.flux;em.line.Hbetadoublenullablee_FHb? Error in flux of Hbeta emission line (e_F_Hbeta)mW.m**-2stat.errordoublenullableFHblim? Upper-limit flux of Hbeta (if no fitting was performed) (F_Hbeta_lim)mW.m**-2phot.flux;em.line.HbetadoublenullableFOIII? Flux of [OIII]5007 emission line (F_OIII)mW.m**-2phot.flux;spect.linedoublenullablee_FOIII? Error in flux of [OIII]5007 emission line (e_F_OIII)mW.m**-2stat.errordoublenullableFOIIIlim? Upper-limit flux of [OIII]5007 (if no fitting was performed) (F_OIII_lim)mW.m**-2phot.fluxdoublenullableFOIIadj? Flux of [OII] emission line adjusted for aperture effect (F_OII_adj) (5)mW.m**-2phot.flux;spect.linedoublenullablee_FOIIadj? Error in flux of [OII] emission line adjusted for aperture effect (e_F_OII_adj) (5)mW.m**-2stat.errordoublenullableFHbadj? Flux of Hbeta emission line adjusted for aperture effect (F_Hbeta_adj) (5)mW.m**-2phot.flux;em.line.Hbetadoublenullablee_FHbadj? Error in flux of Hbeta emission line adjusted for aperture effect (e_F_Hbeta_adj) (5)mW.m**-2stat.errordoublenullableFHbadjlim? Upper-limit flux of Hbeta adjusted for aperture effect (if no fitting was performed) (F_Hbeta_lim_adj) (4)mW.m**-2phot.flux;em.line.HbetadoublenullableFOIIIadj? Flux of [OIII]5007 emission line adjusted for aperture effect (F_OIII_adj) (5)mW.m**-2phot.flux;spect.linedoublenullablee_FOIIIadj? Error in flux of [OIII]5007 emission line adjusted for aperture effect (e_F_OI )5)II_adj) (5)mW.m**-2stat.errordoublenullableFOIIIadjlim? Upper-limit flux of [OIII]5007 adjusted for aperture effect (if no fitting was performed) (F_OIII_lim_adj) (4)mW.m**-2phot.fluxdoublenullableFHaabs? Flux of Halpha emission line adjusted and corrected for absorption (F_Halpha_abs) (3)mW.m**-2phot.flux;em.line.Halphadoublenullablee_FHaabs? Error in flux of Halpha emission line adjusted and corrected for absorption (e_F_Halpha_abs) (3)mW.m**-2stat.errordoublenullableFHbabs? Flux of Hbeta emission line adjusted and corrected for absorption (F_Hbeta_abs)mW.m**-2phot.flux;em.line.Hbetadoublenullablee_FHbabs? Error in flux of Hbeta emission line adjusted and corrected for absorption (e_F_Hbeta_abs)mW.m**-2stat.errordoublenullableFHbabslim? Upper-limit flux of Hbeta adjusted and corrected for absorption (if no fitting was performed) (F_Hbeta_lim_abs)mW.m**-2phot.flux;em.line.HbetadoublenullableFNII6548ec? Flux of [NII]6548 emission line adjusted and corrected for absorptions and extinction (F_NII6548_extinc) (3)mW.m**-2phot.flux;spect.linedoublenullablee_FNII6548ec? Error in flux of [NII]6548 emission line adjusted and corrected for absorptions and extinction (e_F_NII6548_extinc) (3)mW.m**-2stat.errordoublenullableFHaec? Flux of Halpha emission line adjusted and corrected for absorptions and extinction (F_Halpha_extinc)mW.m**-2phot.flux;em.line.Halphadoublenullablee_FHaec? Error in flux of Halpha emission line adjusted and corrected for absorptions and extinction (e_F_Halpha_extinc) (3)mW.m**-2stat.errordoublenullableFNII6583ecFlux of [NII]6583 emission line adjusted and corrected for absorptions and extinction (F_NII6583_extinc) (3)mW.m**-2phot.flux;spect.linedoublee_FNII6583ecError in flux of [NII]6583 emission line adjusted and corrected for absorptions and extinction (e_F_NII6583_extinc) (3)mW.m**-2stat.errordoubleFOIIec? Flux of [OII] emission line adjusted and corrected for absorptions and extinction (F_OII_extinc)mW.m**-2phot.flux;spect.linedoublenullablee_FOIIec? Error in flux of [OII] emission line adjusted and corrected for absorptions and extinction (e_F_OII_extinc)mW.m**-2stat.errordoublenullableFHbec? Flux of Hbeta emission line adjusted and corrected for absorptions and extinction (F_Hbeta_extinc)mW.m**-2phot.flux;em.line.Hbetadoublenullablee_FHbec? Error in flux of Hbeta emission line adjusted and corrected for absorptions and extinction (e_F_Hbeta_extinc)mW.m**-2stat.errordoublenullableFHbeclim? Upper-limit flux of Hbeta adjusted and corrected for absorptions and extinction (if no fitting was performed) (F_Hbeta_lim_extinc)mW.m**-2phot.flux;em.line.HbetadoublenullableFOIIIec? Flux of [OIII]5007 emission line adjusted and corrected for absorptions and extinction (F_OIII_extinc)mW.m**-2phot.flux;spect.linedoublenullablee_FOIIIec? Error in flux of [OIII]5007 emission line adjusted and corrected for absorptions and extinction (e_F_OIII_extinc)mW.m**-2stat.errordoublenullableFOIIIeclim? Upper-limit flux of [OIII]5007 adjusted and corrected for absorptions and extinction (if no fitting was performed) (F_OIII_lim_extinc)mW.m**-2phot.fluxdoublenullableFluxadjfacOII? Flux adjustment factor for [OII] emission line (flux_adj_factor_OII) (5)instr.paramdoublenullableFluxadjfacHb? Flux adjustment factor for Hbeta emission line (flux_adj_factor_Hbeta) (5)instr.paramdoublenullableFluxadjfacOIII? Flux adjustment factor for [OIII]5007 emission line (flux_adj_factor_OIII) (5)instr.paramdoublenullableEWabsHaCSP? Equivalent width of Halpha line obtained from CSP (EW_abs_Halpha_CSP)0.1nmspect.line.eqWidthfloatnullableEWabsHbCSP? Equivalent width of Hbeta line obtained from CSP (EW_abs_Hbeta_CSP)0.1nmspect.line.eqWidthfloatnullableE(B-V)Balmer? Balmer decrement- derived color excess of the stellar continuum (E_B_V_Balmer)phot.color.excessdoublenullableE(B-V)CSP? Color excess of the stellar continuum obtained from CSP (E_B_V_CSP)phot.color.excessdoublenullableE(B-V)used? Color excess of the stellar continuum used to apply correction of extinction (E_B_V_used)phot.color.excessdoublenullableD4000? D4000 break index (D4000)meta.code;spect.indexdoublenullablee_D4000? Error in D4000 break index (e_D4000)stat.errordoublenullableMetN2IC? N2 metallicity (12+log(O/H)) from inverse convolution (Met_N2_InvConv) (3)phys.abund.Zdoublenullableb_MetN2ICLower value of N2 metallicity (12+log(O/H)) from inverse convolution (Met_N2_InvConv_d) (3)phys.abund.Z;stat.mindoubleB_MetN2ICUpper value of N2 metallicity (12+log(O/H)) from inverse convolution (Met_N2_InvConv_u) (3)phys.abund.Z;stat.maxdoubleMetP05? P05 metallicity (12+log(O/H)) (Met_P05)phys.abund.Zdoublenullablee_MetP05? Error in P05 metallicity (12+log(O/H)) (e_Met_P05)stat.errordoublenullableMetZ94? Z94 metallicity (12+log(O/H)) (Met_Z94)phys.abund.Zdoublenullablee_MetZ94? Error in Z94 metallicity (12+log(O/H)) (e_Met_Z94)stat.errordoublenullableMetM91? M91 metallicity (12+log(O/H)) (Met_M91)phys.abund.Zdoublenullablee_MetM91? Error in M91 metallicity (12+log(O/H)) (e_Met_M91)stat.errordoublenullableMetPP04? PP04 metallicity (12+log(O/H)) (Met_PP04)phys.abund.Zdoublenullablee_MetPP04? Error in PP04 metallicity (12+log(O/H)) (e_Met_PP04)stat.errordoublenullableMetT04? T04 metallicity (12+log(O/H)) (Met_T04)phys.abund.Zdoublenullablee_MetT04? Error in T04 metallicity (12+log(O/H)) (e_Met_T04)stat.errordoublenullableSFRHa? Halpha star formation rate (Kennicutt & Evans, 2012ARA&A..50..531K) (SFR_Ha)solMass/yrmeta.iddoublenullablee_SFRHa? Error in Halpha star formation rate based on Halpha (Kennicutt & Evans, 2012ARA&A..50..531K) (e_SFR_Ha)solMass/yrstat.errordoublenullableSFRHb? Hbeta star formation rate based (Kennicutt & Evans, 2012ARA&A..50..531K) (SFR_Hbeta)solMass/yrmeta.iddoublenullablee_SFRHb? Error in Hbeta star formation rate based (Kennicutt & Evans, 2012ARA&A..50..531K) (e_SFR_Hbeta)solMass/yrstat.errordoublenullableSFROIIZ94? [OII] star formation rate corrected by Z94 (Kewley+2004) (SFR_OII_Z94)solMass/yrphys.SFRdoublenullablee_SFROIIZ94? Error in [OII] star formation rate corrected by Z94 (Kewley+2004) (e_SFR_OII_Z94)solMass/yrstat.errordoublenullableSFROIIM91? [OII] star formation rate corrected by M91 (Kewley et al. 2004AJ....127.2002K) (SFR_OII_M91)solMass/yrphys.SFRdoublenullablee_SFROIIM91? Error in [OII] star formation rate corrected by M91 (Kewley, 2004AJ....127.2002K) (e_SFR_OII_M91)solMass/yrstat.errordoublenullableDclusterasCluster-centric projected distance in arcsec (D_cluster_arcsec) (6)arcsecpos.angDistancedoubleDclusterMpcCluster-centric projected distance in Mpc (D_cluster_Mpc) (6)Mpcpos.distancedoublesigma5Local density estimated to the 5th neighbor (sigma5) (6)Mpc**-2src.densitydoublesigma10Local density estimated to the 10th neighbor (sigma10) (6)Mpc**-2src.densitydoubleisAGNSP15True/False flag for AGN activity (isAGN_SP15) (1)meta.codefloatisBLAGNSP15True/False flag for broad-line AGN (isBLAGN_SP15) (1)meta.codefloatisAGNBPT[0/1]? True/False flag for AGN activity based on BPT (Kauffmann+2003); NaN if not conclusive (isAGN_BPT)meta.codefloatnullableisSFGMOS[0/1]True/False flag for star-forming galaxies based on BPT and EWalphaN2; NaN if not conclusive (isSFG_MOS)meta.codefloatisAGNMOS[0/1]True/False flag for AGN activity based on BPT and EWalphaN2; NaN if not conclusive (isAGN_MOS)meta.codefloatisCompMOS[0/1]? True/False flag for composite galaxies based on BPT and EWalphaN2; NaN if not conclusive (isComposite_MOS)meta.codefloatnullableisOutlier[0/1] True/False flag for outlier galaxies (TF redshift not confident) (is_Outlier)meta.codefloatQualIC[1/6] Quality criterion of inverse convolution (Quality_InvConv) (3)meta.code.qualintStructureKinematical structure in which the galaxy is located (Structure) (4)meta.notecharFlagE(B-V)Flag indicating the source of E(B_V_used: "Balmer" for Balmer decrement, "CSP" for CSP (flag_EBV)meta.code.errorchar