J/MNRAS/521/1292ivo://CDS.VizieR/J/MNRAS/521/1292CDSPerez-Millan D.Fritz J.Gonzalez-Lopezlira R.A.Moretti A.,Cervantes Sodi B.Vulcani B.Gullieuszik M.Bruzual G.Charlot S.,Bettoni D.2026-06-12T15:16:35Z2026-06-12T15:48:14ZCDS support team

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

cds-question@unistra.frgalaxiesgalaxy-groupsgalaxy-clustersastrometryredshiftedstar-forming-regionsstellar-massesextinctionstellar-agesabsolute-magnitudephotometryspectroscopyvisible-astronomyinfrared-astronomyx-ray-sourcesgalaxy-kinematicsgalaxy-classification-systemsThe observed properties of galaxies are strongly dependent on both their total stellar mass and their morphology. Furthermore, the environment is known to play a strong role in shaping them. The galaxy population in the local Universe that is located in virialized clusters is found to be red, poorly star-forming, and mostly composed of early morphological types. Towards a holistic understanding of the mechanisms that drive galaxy evolution, we exploit the spectrophotometric data from the WINGS and OmegaWINGS local galaxy cluster surveys, and study the role of both the local and the large-scale environments. We attempt to disentangle their effects from the intrinsic characteristics of the galaxies, in shaping the star formation activity at fixed morphological type and stellar mass. Using a sample of field galaxies from the same surveys for comparison, we analyse the effects of the environment, embodied by the local density, clustercentric distance, and close neighbours, respectively, on the star formation histories of cluster galaxies. We find that local effects have a more relevant impact on galaxy stellar properties than the large-scale environment, and that morphology needs to be taken into account to pinpoint the mechanisms that are driving the influence of clusters in galaxy evolution.2023MNRAS.521.1292Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/521/1292CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/432/3141 : Morphological classification of PM2GC galaxies (Calvi+,2013)J/MNRAS/420/926 : Morphology of galaxies in WINGS clusters (Fasano+, 2012)J/MNRAS/416/727 : Padova-Millennium Galaxy and Group Catalogue (Calvi+, 2011)J/MNRAS/318/333 : Extended ROSAT Bright Cluster Sample (Ebeling+ 2000)J/MNRAS/301/881 : The ROSAT brightest cluster sample - I. (Ebeling+, 1998)J/MNRAS/281/799 : XBACs, the sample (Ebeling+, 1996)J/A+A/607/A81 : Properties of the sample of clusters (Biviano+, 2017)J/A+A/599/A81 : OmegaWINGS local clusters of galaxies redshiftsJ/A+A/599/A83 : ELG and AGN in WINGS clusters (Marziani+, 2017)J/A+A/581/A41 : OmegaWINGS BV photometry of galaxy clustersJ/A+A/566/A32 : Equivalent widths of WINGS galaxies (Fritz+, 2014)J/A+A/497/667 : WINGS: Deep optical phot. of 77 nearby clustersJ/A+A/495/707 : WINGS spectroscopy of 48 galaxy clusters (Cava+, 2009)J/ApJ/949/73 : Galaxy morphologies and local densities from WINGSJ/ApJ/927/91 : Stripping & unwinding galaxies from WINGS surveysJ/ApJS/219/8 : SFR for WISE + SDSS spectroscopic galaxies (Chang+, 2015)J/AJ/151/78 : Jellyfish galaxy candidates in galaxy clustershttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/521/1292https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/521/1292http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/521/1292https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/521/1292https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/521/1292http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/521/1292GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/521/1292/tablec1 (*Basic properties of the WINGS/OmegaWINGS clusters sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/521/1292/tablec1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/521/1292/tablec1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/521/1292/tablec1?GETtext/xml+votable180.050000true159.97625-8.61111110.005555555555555556Cone search capability for table J/MNRAS/521/1292/cluster (Astrometrics and physical properties as ages, masses and SFRs of WINGS cluster galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/521/1292/cluster?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/521/1292/cluster?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/521/1292/cluster?GETtext/xml+votable180.050000true0.13567-35.899410.005555555555555556Cone search capability for table J/MNRAS/521/1292/field (Astrometrics and physical properties as ages, masses and SFRs of WINGS field galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/521/1292/field?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/521/1292/field?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/521/1292/field?GETtext/xml+votable180.050000true0.12561-35.968330.0055555555555555565/4123 4191 4504 5120 6159 6683 6692 8412 10959 6/663 1003 1006 2186 5030 5305 5370 6002 6223 7011 8268 8440 8442 8648 8788 9776 9943 9983 10306-10307 10311-10313 12118 12121 12304 15085 15096 16397 16399 16408 16410 16421 16423 16432 16434 16713 17236-17237 17239 17448 17450 17920 17922 18009 18011-18012 18014 18035 18235 18238 18321 18324 18411 18605-18607 18616 18618 18620 18622-18623 18859 18862 18937 18939 18964-18965 19119 19128 19130-19131 19201 19204 19501 19608 19993 20021 20072 20082-20083 20361 20484 20706 21152 24619 24622 24943 24954 25031 25042-25043 25048-25049 26729 26731 26776-26777 27207 27213 27218 27224 28005 32746 33233-33235 33238 33240-33241 33605 33622 33625 33627-33630 33652 34783 34804-34805 39055 39066 39077 39079 39088 40777 40803 40808-40809 40811-40812 43825 43827-43828 43830 43833 43835 43921 43924 43937-43939 43942 43944-43945 43947-43950 43977 45813 45962 45975 45981 45983-45986 46018 46024 46649 46652-46654 46910-46911 46996-46997 48583 48589 48594-48595 48600https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/521/1292?format=asciiX-rayOpticalInfrareddefaultJ/MNRAS/521/1292/tablec1*Basic properties of the WINGS/OmegaWINGS clusters samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster field namemeta.id;meta.maincharCavaDisplay the WINGS spectroscopy of 48 galaxy clusters of Cava et al. 2009A&A...495..707C, Cat. J/A+A/495/707meta.ref.urlcharVarelaDisplay the WINGS: Deep optical phot. of 77 nearby clusters of Varela et al. 2009A&A...497..667V, Cat. J/A+A/497/667meta.ref.urlcharGullieuszik15Display OmegaWINGS BV photometry of galaxy clusters of Gullieuszik et al. 2015A&A...581A..41G, Cat. J/A+A/581/A41meta.ref.urlcharMorettiDisplay OmegaWINGS local clusters of galaxies redshifts od Moretti et al. 2017A&A...599A..81M, Cat. J/A+A/599/A81meta.ref.urlcharBivianoDisplay Properties of the sample of clusters of Biviano et al. 2017A&A...607A..81B, Cat. J/A+A/607/A81meta.ref.urlcharGullieuszik20Display GASP cluster data of Gullieuszik et al. 2020ApJ...899...13G, Cat. J/ApJ/899/13meta.ref.urlcharzThe mean redshiftsrc.redshiftdoublesigma? The velocity dispersion from data Biviano et al. (2017A&A...607A..81B, Cat. J/A+A/607/A81) and Gullieuszik et al. (2020ApJ...899...13G, Cat. J/ApJ/899/13)km/sphys.veloc.dispersionintnullableR200? The virial radiusMpcphys.size.radiusfloatnullablelogLX? The X-ray luminosity taken from the ROSAT All-Sky Surveylog(1e-07W)phys.luminosity;em.X-rayfloatnullableWingsFlag to indicates if the cluster was observed in spectroscopy with WINGSmeta.codecharOWingsFlag to indicates if the cluster was observed in spectroscopy with Omega Wingsmeta.codecharSimbadNameSimbad column added by the CDSmeta.idcharnullableSinopsisFlag to whether WINGS/OmegaWINGS spectra have sufficient signal-to-noise ratio to run the sinopsis codemeta.codechar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/MNRAS/521/1292/clusterAstrometrics and physical properties as ages, masses and SFRs of WINGS cluster galaxiesSimbadSimbad column added by the CDSmeta.ref.urlcharBmagApparent magnitude with automatic aperture in B-band (Bauto)magphot.mag;em.opt.BfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintWINGSWINGS identifier designation as WINGSJHHMMSS.ss+DDMMSS.s (WINGS_ID)meta.id;meta.maincharRAJ2000Right ascension (J2000) (RAJ2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) (DECJ2000)degpos.eq.dec;meta.mainzgalRedshift of the galaxies (z_gal)src.redshiftdoubleDLDistance luminosity (Lum_dist)Mpcpos.distancefloatrChiReduced chi squared of the SINOPSIS model spectral profile fit (redchi)stat.fit.chi2;spect.line.profile;meta.modelleddoubleAVyExtinction of the youngest stellar populations as age <=2*10^7 yr (Av_y)magphys.absorptionfloatAvAverage extinction value for all the stellar populations (Av)magphys.absorption;stat.meanfloatSFR1SFR in first age-bin 0-19.95 Myr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR1) (G1)solMass/yrphys.SFRfloatSFR2SFR in second age-bin 19.95-571.5 Myr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR2) (G1)solMass/yrphys.SFRfloatSFR3SFR in third age-bin from 0.5715-5.754 Gyr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR3) (G1)solMass/yrphys.SFRfloatSFR4SFR in fourth age-bin from 5.754-tu Gyr as described in sect. 3 were selected based on the presence and intensity of stellar population features (SFR4) (G1)solMass/yrphys.SFRfloatM*a3Stellar mass, calculated according to definition n.3 of the SFR3, normalized to aperture magnitude or spectrum (AMass3)solMassphys.massdoubleTotM*3Total stellar mass calculated according to definition n.3 of the SFR3 (TotMass3)solMassphys.massdoubleM*a2Stellar mass, calculated according to definition n.2 of the SFR2, normalized to aperture magnitude or spectrum (AMass2)solMassphys.massdoubleTotM*2Total stellar mass calculated according to definition n.2 of the SFR2 (TotMass2)solMassphys.massdoubleM*a1Stellar mass, calculated according to definition n.1 of the SFR1, normalized to aperture magnitude or spectrum (AMass1)solMassphys.massdoubleTotM*1Total stellar mass calculated according to definition n.1 of the SFR1 (TotMass1)solMassphys.massdoublelogAgelwVLogarithm of the luminosity-weighted age in V-band (lVwage)log(yr)time.agefloatlogAgemwLogarithm of the mass-weighted age (mwage)log(yr)time.agefloatHbThe H{Beta} index (Hb)0.1nmspect.index;em.line.HbetafloatHaThe H{alpha} index (Ha)0.1nmspect.index;em.line.HalphafloatD4000The D4000 4000{AA} break index (D4000)spect.indexfloatDn4000The Dn4000 spectral indicator (Dn4000)spect.indexfloatSNRSignal to noise ratio (SNR)stat.snrfloatBfibMagAbsolute magnitude with fiber aperture in B-band (ABS_B_fib)magphot.magfloatVfibMagAbsolute magnitude with fiber aperture in V-band (ABS_V_fib)magphot.magfloatVmagApparent magnitude with automatic aperture in V-band (Vauto)magphot.mag;em.opt.VfloatVfibmagApparent magnitude with fiber aperture in V-band (V_fib)magphot.mag;em.opt.VfloatBfibmagApparent magnitude with fiber aperture in B-band (B_fib)magphot.mag;em.opt.BfloatVtotMagTotal absolute magnitude in V-band (ABS_V_tot)magphot.magfloatBtotMagTotal absolute magnitude in B-band (ABS_B_tot)magphot.magfloatzclRedshift of the cluster (z_cl)src.redshift;pos.heliocentricdoublesigmaThe cluster velocity dispersion {sigma}_cl_ (sigma_cl)km/sphys.veloc.dispersionfloatR200The viral radius as defined by equation 1 of the section 2.3 (r200) (1)Mpcphys.size.radiusfloatlogLXThe X-ray luminosity mostly taken from ROSAT all-sky surveys (logLX)log(1e-07W)phys.luminosity;em.X-rayfloatRXprojThe clustercentric distance radius is calculated in projection to the centre of the cluster in the X-ray emission (RXproj)Mpcpos.distancedoubleMorphFlag for cluster morphology of neighbour galaxies as early and late types (neigh_morph)meta.codecharRRvThe cluster RRv quantity (RRv)stat.paramfloatGullieuszik15Display OmegaWINGS BV photometry of galaxy clusters of Gullieuszik et al. 2015A&A...581A..41G, Cat. J/A+A/581/A41meta.ref.urlcharMorettiDisplay OmegaWINGS local clusters of galaxies redshifts od Moretti et al. 2017A&A...599A..81M, Cat. J/A+A/599/A81meta.ref.urlcharClusterCluster designation as ANNNN (Cluster)meta.id.parentcharJ/MNRAS/521/1292/fieldAstrometrics and physical properties as ages, masses and SFRs of WINGS field galaxiesSimbadSimbad column added by the CDSmeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000) (RAJ2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) (DECJ2000)degpos.eq.dec;meta.mainzgalRedshift of the galaxies (z_gal)src.redshiftdoubleDLDistance luminosity (Lum_dist)Mpcpos.distancefloatrChiReduced chi squared of the SINOPSIS model spectral profile fit (redchi)stat.fit.chi2;spect.line.profile;meta.modelleddoubleAVyExtinction of the youngest stellar populations as age <=2*10^7 yr (Av_y)magphys.absorptionfloatAvAverage extinction value for all the stellar populations (Av)magphys.absorption;stat.meanfloatSFR1SFR in first age-bin from 0 to 19.95 Myr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR1) (G1)solMass/yrphys.SFRfloatSFR2SFR in second age-bin from 19.95 to 571.5 Myr as described in sect. 3 were selected based on presence and intensity of stellar population features (SFR2) (G1)solMass/yrphys.SFRfloatSFR3SFR in third age-bin from 0.5715-5.754 Gyr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR3) (G1)solMass/yrphys.SFRfloatSFR4SFR in fourth age-bin from 5.754-tu Gyr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR4) (G1)solMass/yrphys.SFRfloatM*a3Stellar mass, calculated according to definition n.3 of the SFR3, normalized to aperture magnitude or spectrum (AMass3)solMassphys.massdoubleTotM*3Total stellar mass calculated according to definition n.3 of the SFR3 (TotMass3)solMassphys.massdoubleM*a2Stellar mass, calculated according to definition n.2 of the SFR2, normalized to aperture magnitude or spectrum (AMass2)solMassphys.massdoubleTotM*2Total stellar mass calculated according to definition n.2 of the SFR2 (TotMass2)solMassphys.massdoubleM*a1Stellar mass, calculated according to definition n.1 of the SFR1, normalized to aperture magnitude or spectrum (AMass1)solMassphys.massdoubleTotM*1Total stellar mass calculated according to definition n.1 of the SFR1 (TotMass1)solMassphys.massdoublelogAgelwVLogarithm of the luminosity-weighted age in V-band (lVwage)log(yr)time.agefloatlogAgemwLogarithm of the mass-weighted age (mwage)log(yr)time.agefloatHbThe H{Beta} index (Hb)0.1nmspect.index;em.line.HbetafloatHaThe H{alpha} index (Ha)0.1nmspect.index;em.line.HalphafloatD4000The D4000 4000{AA} break index (D4000)spect.indexfloatDn4000The Dn4000 spectral indicator (Dn4000)spect.indexfloatSNRSignal to noise ratio (SNR)stat.snrfloatBfibMagAbsolute magnitude with fiber aperture in B-band (ABS_B_fib)magphot.magfloatVfibMagAbsolute magnitude with fiber aperture in V-band (ABS_V_fib)magphot.magfloatVmagApparent magnitude with automatic aperture in V-band (Vauto)magphot.mag;em.opt.VfloatVfibmagApparent magnitude with fiber aperture in V-band (V_fib)magphot.mag;em.opt.VfloatBmagApparent magnitude with automatic aperture in B-band (Bauto)magphot.mag;em.opt.BfloatBfibmagApparent magnitude with fiber aperture in B-band (B_fib)magphot.mag;em.opt.BfloatVtotMagTotal absolute magnitude in V-band (ABS_V_tot)magphot.magfloatBtotMagTotal absolute magnitude in B-band (ABS_B_tot)magphot.magfloatWINGSWINGS identifier desingation as WINGSJHHMMSS.ss+DDMMSS.s (WINGS_ID)meta.id;meta.maincharGullieuszik15Display OmegaWINGS BV photometry of galaxy clusters of Gullieuszik et al. 2015A&A...581A..41G, Cat. J/A+A/581/A41meta.ref.urlcharMorettiDisplay OmegaWINGS local clusters of galaxies redshifts od Moretti et al. 2017A&A...599A..81M, Cat. J/A+A/599/A81meta.ref.urlcharClusterCluster designation as ANNNN (Cluster)meta.id.parentchar