J/MNRAS/485/586ivo://CDS.VizieR/J/MNRAS/485/586doi:10.26093/cds/vizier.74850586CDSRodriguez-Munoz L.Rodighiero G.Mancini C.Perez-Gonzalez P.G.,Rawle T.D.Egami E.Mercurio A.Rosati P.Puglisi A.Franceschini A.,Balestra I.Baronchelli I.Biviano A.Ebeling H.Edge A.C.,Enia A.F.M.Grillo C.Haines C.P.Iani E.Jones T.Nonino M.,Valtchanov I.Vulcani B.Zemcov M.2024-08-19T20:17:59Z2022-10-20T14:30:35ZCDS support team

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

cds-question@unistra.frgalaxiesgalaxy-clusterscatalogsultraviolet-photometryinfrared-photometryWe quantify the star formation (SF) in the inner cores (R/R_200_~<0.3) of 24 massive galaxy clusters at 0.2~<z~<0.9 observed by the Herschel Lensing Survey and the Cluster Lensing and Supernova survey with Hubble. These programmes, covering the rest-frame ultraviolet to far-infrared regimes, allow us to accurately characterize stellar mass-limited (M_*_>10^10^M_{sun}_) samples of star-forming cluster members (not)-detected in the mid- and/or far-infrared. We release the catalogues with the photometry, photometric redshifts, and physical properties of these samples. We also quantify the SF displayed by comparable field samples from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey. We find that in intermediate-z cluster cores, the SF activity is suppressed with respect the field in terms of both the fraction (F) of star-forming galaxies (SFGs) and the rate at which they form stars (SFR and sSFR=SFR/M_*_). On average, the F of SFGs is a factor ~2 smaller in cluster cores than in the field. Furthermore, SFGs present average SFR and sSFR typically ~0.3dex smaller in the clusters than in the field along the whole redshift range probed. Our results favour long time-scale quenching physical processes as the main driver of SF suppression in the inner cores of clusters since z~0.9, with shorter time-scale processes being very likely responsible for a fraction of the missing SFG population.2019MNRAS.485..586Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/485/586CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/485/586https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/485/586http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/485/586https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/485/586https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/485/586http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/485/586GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/485/586/table1 (Description of the galaxy cluster sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/485/586/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/485/586/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/485/586/table1?GETtext/xml+votable180.050000true42.0141667-3.52913890.0055555555555555566/6383 6441 6539 7904 8921 9052 9476 9498 17457 19097 22771 23173 25451 25675 26177 27075 28448 28535 34793 36846 46474 48076 48423 490123.2031150387835462e-22 6.185923063528282e-20https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/485/586?format=asciiUVInfrareddefaultJ/MNRAS/485/586/table1Description of the galaxy cluster sampleSimbadNameSimbad column added by the CDSmeta.idcharnullablesigclVelocity dispersion {sigma}_cl_ (3)km/sphys.veloc.dispersionintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.maincharf_z[*] Flag on redshift (2)meta.codecharRAJ2000Right ascension (J2000) (1)pos.eq.ra;meta.mainDEJ2000Declination (J2000) (1)pos.eq.dec;meta.mainzRedshift from Postman et al. (2012ApJS..199...25P, Cat. J/ApJS/199/25)src.redshiftfloatE_sigcl? Upper error on sigclkm/sstat.error;stat.maxintnullablee_sigcl? Lower error on sigclkm/sstat.errorintnullabler_sigclReferences for sigcl (5)meta.ref;pos.framecharR200Radius within which the mean density is 200 times the critical density at the redshift where the cluster is located (4)kpcphys.size.radiusintE_R200? Upper error on R200kpcstat.error;stat.maxintnullablee_R200? Lower error on R200kpcstat.errorintnullabler_R200References for R200 (5)meta.ref;pos.framecharl_SFRUVLimit flag on SFRUVmeta.code.errorcharSFRUV? SF activity of the BCG as quantified through the emission of the UV, corrected for extinction (Fogarty et al. 2015ApJ...813..117F)solMass/yrphys.SFRfloatnullablee_SFRUV? Error on SFRUVsolMass/yrstat.errorfloatnullableSFRFIR? SF activity of the BCG as quantified through the emission of the FIR (Rawle et al. 2012ApJ...747...29R)solMass/yrphys.SFRfloatnullablee_SFRFIR? Error on SFRFIRsolMass/yrstat.errorfloatnullableCCC tracer C parameter as published by Donahue et al. 2016ApJ...819...36Dmeta.ref;stat.paramfloatNzpec? Number of spectroscopic redshifts within the area covered by the CLASH catalogue (~0.0015deg^2^)meta.numberintnullabler_NzpecReferences for Nzpec (5)meta.ref;pos.framecharJ/MNRAS/485/586/table2Overview of the photometric bands used in this workProjectName of the project to which the data belongs (1)meta.id;obscharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBandName of the instrument and observing bandmeta.id;instr.bandpasscharwleffEffective wavelength of the filterumem.wl.effective;instr.filterdoubleFWHMMedian FWHM of the PSFarcsecinstr.bandwidthfloatJ/MNRAS/485/586/table3Limiting fluxes (5{sigma}) of the Spitzer and Herschel photometric catalogues used in this workrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.maincharFIRAC3.6Spitzer/IRAC 3.6um limiting flux (5{sigma})uJyphot.mag;em.IR.3-4umfloatFIRAC4.5Spitzer/IRAC 4.5um limiting flux (5{sigma})uJyphot.mag;em.IR.4-8umfloatFIRAC5.8? Spitzer/IRAC 5.8um limiting flux (5{sigma})uJyphot.flux.density;em.IR.4-8umfloatnullableFIRAC8.0? Spitzer/IRAC 8.0um limiting flux (5{sigma})uJyphot.flux.density;em.IR.8-15umfloatnullableFMIPS24? Spitzer/MIPS 24um limiting flux (5{sigma})uJyphot.flux.density;em.IR.15-30umfloatnullableFPACS100Herschel/PACS 100um limiting flux (5{sigma})mJyphot.flux.density;em.IR.60-100umfloatFPACS160Herschel/PACS 160um limiting flux (5{sigma})mJyphot.flux.density;em.mm.1500-3000GHzfloatFSPIRE250Herschel/SPIRE 250um limiting flux (5{sigma})mJyphot.flux.density;em.mm.750-1500GHzfloatFSPIRE350Herschel/SPIRE 350um limiting flux (5{sigma})mJyphot.flux.density;em.mm.750-1500GHzfloatFSPIRE500Herschel/SPIRE 500um limiting flux (5{sigma})mJyphot.flux.density;em.mm.400-750GHzfloatJ/MNRAS/485/586/table4Summary of some of the quantities used for the identification of cluster members and an evaluation of the techniqueIDCluster IDmeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNzNumber of spectroscopic members (1)meta.numberintsigNMADNormalized median absolute deviation of the difference between the zphot and the zspec (2)stat.stdev;em.wl.central;stat.medianfloatnNumber of sigNMAD to be used in the integration of the P(z) (3)meta.numberintPthrMembership probability thresholdmeta.code.memberfloatKCompleteness level (per cent)meta.noteintIFraction of interlopers (per cent)stat.fit.paramintJ/MNRAS/485/586/table5Number of galaxies selected with the different criteria used to build the final samples of star-forming cluster members (R/R_200_<0.1), and average SF activity indicatorsMFIRTotal number of cluster members without SFRTIR cutmeta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.maincharMembcutNumber of cluster members with a detection at a level >3{sigma} in IRAC 4.5um and M*>10^10^M_{sun}_meta.numberintMembNumber of cluster members without the M* cutmeta.numberintUVJSFNumber of galaxies selected as star-forming using the UVJ diagram and/or detected in the MIR and/or FIR (M>10^10^M_{sun}_), what we call the UVJ-SF samplemeta.numberintMFIRcutCluster members with M*>10^10^M_{sun}_ detected in the MIR and/or FIR with SFRTIR>10M_{sun}_/yr what we call MFIR samplemeta.numberintFUVJSFFraction of UVJ-SF galaxies, obtained using as reference the number of cluster members with M*>10^10^M_{sun}_meta.numberfloate_FUVJSFError on FUVJSFstat.errorfloatFMFIR? Fraction of M-FIR galaxies, obtained using as reference the number of cluster members with M*>10^10^M_{sun}_meta.numberfloatnullablee_FMFIR? Error on FMFIRstat.errorfloatnullableMUVJSFStellar mass of the UVJ-SF samplelog(solMass)phys.massfloatE_MUVJSFUpper error on MUVJSF (84th quantile)log(solMass)stat.error;stat.maxfloate_MUVJSFLower error on MUVJSF (16th quantile)log(solMass)stat.errorfloatMMFIR? Stellar mass of the M-FIR samplelog(solMass)phys.massfloatnullableSFRUVJSFTotal SFR for the UVJ-SF sample obtained as the addition of the SFRTIR and the SFRUV when the former is available, and the SFRUVcorr in the rest of the cases (1)log(solMass.yr**-1)phys.SFRfloatE_SFRUVJSFUpper error on SFRUVJSF (84th quantile)log(solMass.yr**-1)stat.error;stat.maxfloate_SFRUVJSFLower error on SFRUVJSF (16th quantile)log(solMass.yr**-1)stat.errorfloatSFRMFIR? Total SFR for the M-FIR sample obtained as the addition of the SFRTIR and the SFRUV (1)log(solMass.yr**-1)phys.SFRfloatnullablesSFRUVJSFSpecific star formation rate for the UVJ-SF sample (2)log(yr**-1)phys.SFRfloatE_sSFRUVJSFUpper error on sSFRUVJSF (84th quantile)log(yr**-1)stat.error;stat.maxfloate_sSFRUVJSFLower error on sSFRUVJSF (16th quantile)log(yr**-1)stat.errorfloatsSFRMFIR? Specific star formation rate for the M-FIR sample (2)log(yr**-1)phys.SFRfloatnullableJ/MNRAS/485/586/table6Number of galaxies selected with the different criteria used to build the final samples of star-forming cluster members (0.1<R/R_200_<0.2), and average SF activity indicatorse_FUVJSF? Error on FUVJSFstat.errorfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.maincharMembcutNumber of cluster members with a detection at a level >3{sigma} in IRAC 4.5um and M*>10^10^M_{sun}_meta.numberintMembNumber of cluster members without the M* cutmeta.numberintUVJSFNumber of galaxies selected as star-forming using the UVJ diagram and/or detected in the MIR and/or FIR (M>10^10^M_{sun}_), what we call the UVJ-SF samplemeta.numberintMFIRcutCluster members with M*>10^10^M_{sun}_ detected in the MIR and/or FIR with SFRTIR>10M_{sun}_/yr what we call MFIR samplemeta.numberintMFIRTotal number of cluster members without SFRTIR cutmeta.numberintFUVJSF? Fraction of UVJ-SF galaxies, obtained using as reference the number of cluster members with M*>10^10^M_{sun}_meta.numberfloatnullableFMFIR? Fraction of M-FIR galaxies, obtained using as reference the number of cluster members with M*>10^10^M_{sun}_meta.numberfloatnullablee_FMFIR? Error on FMFIRstat.errorfloatnullableMUVJSF? Stellar mass of the UVJ-SF samplelog(solMass)phys.massfloatnullableE_MUVJSF? Upper error on MUVJSF (84th quantile)log(solMass)stat.error;stat.maxfloatnullablee_MUVJSF? Lower error on MUVJSF (16th quantile)log(solMass)stat.errorfloatnullableMMFIR? Stellar mass of the M-FIR samplelog(solMass)phys.massfloatnullableE_MMFIR? Upper error on MMFIR (84th quantile)log(solMass)stat.error;stat.maxfloatnullablee_MMFIR? Lower error on MMFIR (16th quantile)log(solMass)stat.errorfloatnullableSFRUVJSF? Total SFR for the UVJ-SF sample obtained as the addition of the SFRTIR and the SFRUV when the former is available, and the SFRUVcorr in the rest of the cases (1)log(solMass.yr**-1)phys.SFRfloatnullableE_SFRUVJSF? Upper error on SFRUVJSF (84th quantile)log(solMass.yr**-1)stat.error;stat.maxfloatnullablee_SFRUVJSF? Lower error on SFRUVJSF (16th quantile)log(solMass.yr**-1)stat.errorfloatnullableSFRMFIR? Total SFR for the M-FIR sample obtained as the addition of the SFRTIR and the SFRUV (1)log(solMass.yr**-1)phys.SFRfloatnullableE_SFRMFIR? Upper error on SFRMFIR (84th quantile)log(solMass.yr**-1)stat.error;stat.maxfloatnullablee_SFRMFIR? Lower error on SFRMFIR (16th quantile)log(solMass.yr**-1)stat.errorfloatnullablesSFRUVJSF? Specific star formation rate for the UVJ-SF sample (2)log(yr**-1)phys.SFRfloatnullableE_sSFRUVJSF? Upper error on sSFRUVJSF (84th quantile)log(yr**-1)stat.error;stat.maxfloatnullablee_sSFRUVJSF? Lower error on sSFRUVJSF (16th quantile)log(yr**-1)stat.errorfloatnullablesSFRMFIR? Specific star formation rate for the M-FIR sample (2)log(yr**-1)phys.SFRfloatnullableE_sSFRMFIR? Upper error on sSFRMFIR (84th quantile)log(yr**-1)stat.error;stat.maxfloatnullablee_sSFRMFIR? Lower error on sSFRMFIR (16th quantile)log(yr**-1)stat.errorfloatnullableJ/MNRAS/485/586/table7Number of galaxies selected with the different criteria used to build the final samples of star-forming cluster members (0.2<R/R_200_<0.3), and average SF activity indicatorsIDCluster IDmeta.id;meta.mainchare_FUVJSF? Error on FUVJSFstat.errorfloatnullablesSFRUVJSF? Specific star formation rate for the UVJ-SF sample (2)log(yr**-1)phys.SFRfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMembcutNumber of cluster members with a detection at a level >3{sigma} in IRAC 4.5um and M*>10^10^M_{sun}_meta.numberintMembNumber of cluster members without the M* cutmeta.numberintUVJSFNumber of galaxies selected as star-forming using the UVJ diagram and/or detected in the MIR and/or FIR (M>10^10^M_{sun}_), what we call the UVJ-SF samplemeta.numberintMFIRcutCluster members with M*>10^10^M_{sun}_ detected in the MIR and/or FIR with SFRTIR>10M_{sun}_/yr what we call MFIR samplemeta.numberintMFIRTotal number of cluster members without SFRTIR cutmeta.numberintFUVJSF? Fraction of UVJ-SF galaxies, obtained using as reference the number of cluster members with M*>10^10^M_{sun}_meta.numberfloatnullableFMFIR? Fraction of M-FIR galaxies, obtained using as reference the number of cluster members with M*>10^10^M_{sun}_meta.numberfloatnullablee_FMFIR? Error on FMFIRstat.errorfloatnullableMUVJSF? Stellar mass of the UVJ-SF samplelog(solMass)phys.massfloatnullableE_MUVJSF? Upper error on MUVJSF (84th quantile)log(solMass)stat.error;stat.maxfloatnullablee_MUVJSF? Lower error on MUVJSF (16th quantile)log(solMass)stat.errorfloatnullableMMFIR? Stellar mass of the M-FIR samplelog(solMass)phys.massfloatnullableE_MMFIR? Upper error on MMFIR (84th quantile)log(solMass)stat.error;stat.maxfloatnullablee_MMFIR? Lower error on MMFIR (16th quantile)log(solMass)stat.errorfloatnullableSFRUVJSF? Total SFR for the UVJ-SF sample obtained as the addition of the SFRTIR and the SFRUV when the former is available, and the SFRUVcorr in the rest of the cases (1)log(solMass.yr**-1)phys.SFRfloatnullableE_SFRUVJSF? Upper error on SFRUVJSF (84th quantile)log(solMass.yr**-1)stat.error;stat.maxfloatnullablee_SFRUVJSF? Lower error on SFRUVJSF (16th quantile)log(solMass.yr**-1)stat.errorfloatnullableSFRMFIR? Total SFR for the M-FIR sample obtained as the addition of the SFRTIR and the SFRUV (1)log(solMass.yr**-1)phys.SFRfloatnullableE_SFRMFIR? Upper error on SFRMFIR (84th quantile)log(solMass.yr**-1)stat.error;stat.maxfloatnullablee_SFRMFIR? Lower error on SFRMFIR (16th quantile)log(solMass.yr**-1)stat.errorfloatnullableE_sSFRUVJSF? Upper error on sSFRUVJSF (84th quantile)log(yr**-1)stat.error;stat.maxfloatnullablee_sSFRUVJSF? Lower error on sSFRUVJSF (16th quantile)log(yr**-1)stat.errorfloatnullablesSFRMFIR? Specific star formation rate for the M-FIR sample (2)log(yr**-1)phys.SFRfloatnullableE_sSFRMFIR? Upper error on sSFRMFIR (84th quantile)log(yr**-1)stat.error;stat.maxfloatnullablee_sSFRMFIR? Lower error on sSFRMFIR (16th quantile)log(yr**-1)stat.errorfloatnullableJ/MNRAS/485/586/table8Number counts and average properties of field galaxy samplese_FMFIR? Error on FMFIRstat.errorfloatnullableFUVJSF? Fraction of UVJ-SF galaxies, obtained using as reference the number of cluster members with M*>10^10^M_{sun}_meta.numberfloatnullablee_FUVJSF? Error on FUVJSFstat.errorfloatnullableFMFIR? Fraction of M-FIR galaxies, obtained using as reference the number of cluster members with M*>10^10^M_{sun}_meta.numberfloatnullableMUVJSF? Stellar mass of the UVJ-SF samplelog(solMass)phys.massfloatnullableE_MUVJSF? Upper error on MUVJSF (84th quantile)log(solMass)stat.error;stat.maxfloatnullablee_MUVJSF? Lower error on MUVJSF (16th quantile)log(solMass)stat.errorfloatnullableMMFIR? Stellar mass of the M-FIR samplelog(solMass)phys.massfloatnullableE_MMFIR? Upper error on MMFIR (84th quantile)log(solMass)stat.error;stat.maxfloatnullablee_MMFIR? Lower error on MMFIR (16th quantile)log(solMass)stat.errorfloatnullableSFRUVJSF? Total SFR for the UVJ-SF sample obtained as the addition of the SFRTIR and the SFRUV when the former is available, and the SFRUVcorr in the rest of the cases (1)log(solMass.yr**-1)phys.SFRfloatnullableE_SFRUVJSF? Upper error on SFRUVJSF (84th quantile)log(solMass.yr**-1)stat.error;stat.maxfloatnullablee_SFRUVJSF? Lower error on SFRUVJSF (16th quantile)log(solMass.yr**-1)stat.errorfloatnullableSFRMFIR? Total SFR for the M-FIR sample obtained as the addition of the SFRTIR and the SFRUV (1)log(solMass.yr**-1)phys.SFRfloatnullableE_SFRMFIR? Upper error on SFRMFIR (84th quantile)log(solMass.yr**-1)stat.error;stat.maxfloatnullablee_SFRMFIR? Lower error on SFRMFIR (16th quantile)log(solMass.yr**-1)stat.errorfloatnullablesSFRUVJSF? Specific star formation rate for the UVJ-SF sample (2)log(yr**-1)phys.SFRfloatnullableE_sSFRUVJSF? Upper error on sSFRUVJSF (84th quantile)log(yr**-1)stat.error;stat.maxfloatnullablee_sSFRUVJSF? Lower error on sSFRUVJSF (16th quantile)log(yr**-1)stat.errorfloatnullablesSFRMFIR? Specific star formation rate for the M-FIR sample (2)log(yr**-1)phys.SFRfloatnullableE_sSFRMFIR? Upper error on sSFRMFIR (84th quantile)log(yr**-1)stat.error;stat.maxfloatnullablee_sSFRMFIR? Lower error on sSFRMFIR (16th quantile)log(yr**-1)stat.errorfloatnullableIDCluster IDmeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMembcutNumber of cluster members with a detection at a level >3{sigma} in IRAC 4.5um and M*>10^10^M_{sun}_meta.numberintMembNumber of cluster members without the M* cutmeta.numberintUVJSFNumber of galaxies selected as star-forming using the UVJ diagram and/or detected in the MIR and/or FIR (M>10^10^M_{sun}_), what we call the UVJ-SF samplemeta.numberintMFIRcutCluster members with M*>10^10^M_{sun}_ detected in the MIR and/or FIR with SFRTIR>10M_{sun}_/yr what we call MFIR samplemeta.numberintMFIRTotal number of cluster members without SFRTIR cutmeta.numberint