J/MNRAS/501/2430ivo://CDS.VizieR/J/MNRAS/501/2430doi:10.26093/cds/vizier.75012430CDSBeyoro-Amado Z.Sanchez-Portal M.Bongiovanni A.Povic M.Tessema S.B.,Perez-Martinez R.Perez Garcia A.M.Cervino M.Nadolny J.Cepa J.,Gonzalez-Serrano J.I.Pintos-Castro I.2024-08-21T20:17:02Z2023-11-15T08:06:57ZCDS support team

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

cds-question@unistra.frgalaxy-clustersactive-galactic-nucleigalaxiesredshiftedgalaxy-classification-systemsvisible-astronomyAlthough ZwCl0024+1652 galaxy cluster at z~0.4 has been thoroughly analysed, it lacks a comprehensive study of star formation and nuclear activity of its members. With GaLAxy Cluster Evolution (GLACE) survey, a total of 174 H{alpha} emission-line galaxies (ELGs) were detected, most of them having [NII]. We reduced and analysed a set of [OIII] and H{beta} tunable filter (TF) observations within GLACE survey. Using H{alpha} priors, we identified [OIII] and H{beta} in 35 (~20 per cent) and 59 (~34 per cent) sources, respectively, with 21 of them having both emission lines, and 20 having in addition [NII]. Applying BPT-NII diagnostic diagram, we classified these ELGs into 40 per cent star-forming (SF), 55 per cent composites, and 5 per cent LINERs. Star formation rate (SFR) measured through extinction corrected H{alpha} fluxes increases with stellar mass (M_*_), attaining its peak at M_*_~10^9.8^M_{sun}_. We observed that the cluster centre to ~1.3Mpc is devoid of SF galaxies and AGN. Our results suggest that the star formation efficiency declines as the local density increases in the cluster medium. Moreover, the SF and AGN fractions drop sharply towards high-density environments. We observed a strong decline in SF fraction in high M_*_, confirming that star formation is highly suppressed in high-mass cluster galaxies. Finally, we determined that SFR correlates with M_*_ while specific SFR (sSFR) anticorrelates with M_*_, both for cluster and field. This work shows the importance and strength of TF observations when studying ELGs in clusters at higher redshifts. We provide with this paper a catalogue of ELGs with H{beta} and/or [OIII] lines in ZwCl0024+1652 cluster.2021MNRAS.501.2430Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/501/2430CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/591/53 : I photometry of Cl 0024+16 (Treu+, 2003)J/ApJ/671/1503 : Cl 0024+16 and MS 0451-03 spectrophotometry (Moran+, 2007)J/MNRAS/485/1528 : Morphological study of galaxies in ZwCl0024+1652https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/501/2430https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/501/2430http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/501/2430https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/501/2430https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/501/2430http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/501/2430GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/501/2430/tablea1 (Example of the catalogue describing [OIII] and H{beta} emitters in ZwCl0024+1652 cluster)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/501/2430/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/501/2430/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/501/2430/tablea1?GETtext/xml+votable180.050000true6.62322817.24699440.0055555555555555566/19846https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/501/2430?format=asciiOpticaldefaultJ/MNRAS/501/2430/tablea1Example of the catalogue describing [OIII] and H{beta} emitters in ZwCl0024+1652 clusterIDHST? HST identifiermeta.idintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDHaH{alpha} line ID number with subscript O for offset and C for centre positionmeta.id;meta.maincharIDOIIIOIII line ID number with subscript O for offset and C for centre positionmeta.idcharIDHbH{beta} line ID number with subscript O for offset and C for centre positionmeta.idcharRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainRClustercentric distanceMpcpos.distancedoublezOIII? TF redshift measured with [OIII] linesrc.redshift;pos.heliocentricdoublenullablezHb? TF redshift measured with H{beta} linesrc.redshift;pos.heliocentricdoublenullablezHa? TF redshift measured with H{alpha} linesrc.redshift;pos.heliocentricdoublenullablefOIII? [OIII] Flux1e-19W.m**-2phot.fluxdoublenullablefHb? H{beta} flux1e-19W.m**-2phot.flux;spect.linedoublenullableLinesList of emission lines detectedmeta.id;spect.linecharfHa? H{alpha} flux1e-19W.m**-2phot.flux;spect.linedoublenullablefNII? [NII] Flux1e-19W.m**-2phot.fluxdoublenullableEWHb? H{beta} equivalent width0.1nmspect.line.eqWidthfloatnullablelogM*? Logarithm of the stellar masslog(solMass)phys.massdoublenullableELGtypeEmission line galaxy (ELG) type based on Sanchez-Portal et al. (2015A&A...578A..30S, Cat. J/A+A/578/A30) (1)meta.code.classcharBPTclassBPT-NII classification (2)meta.code.classcharMorphBroad morphological class (3)meta.code.classcharr_MorphReference for Morph (4)meta.ref;pos.framechar