J/A+A/678/A145ivo://CDS.VizieR/J/A+A/678/A145doi:10.26093/cds/vizier.36780145CDSMaturi M.Finoguenov A.Lopes P.A.A.Gonzalez Delgado R.M.Dupke R.A.,Cypriano E.S.Carrasco E.R.Diego J.M.Penna-Lima M.Vilchez J.M.,Moscardini L.Marra V.Bonoli S.Rodriguez-Martin J.E.Zitrin A.,Marquez I.Hernan-Caballero A.Jimenez-Teja Y.Abramo R.Alcaniz J.,Benitez N.Carneiro S.Cenarro J.Cristobal-Hornillos D.Ederoclite A.,Lopez-Sanjuan C.Marin-Franch A.Mendes de Oliveira C.Moles M.,Sodre Jr.L.Taylor K.Varela J.Vazquez Ramio H.,Fernandez-Ontiveros J.A.2024-11-28T20:05:22Z2023-10-17T15:48:55ZCDS support team

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

cds-question@unistra.frgalaxy-clusterssurveysredshiftedx-ray-sourcesvisible-astronomySamples of galaxy clusters allow us to better understand the physics at play in galaxy formation and to constrain cosmological models once their mass, position (for clustering studies) and redshift are known. In this context, large optical data sets play a crucial role. We investigate the capabilities of the Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) in detecting and characterizing galaxy groups and clusters. We analyze the data of the miniJPAS survey, obtained with the JPAS-Pathfinder camera and covering 1deg^2^ centered on the AEGIS field to the same depths and with the same 54 narrow band plus 2 broader band near-UV and near-IR filters anticipated for the full J-PAS survey. We use the Adaptive Matched Identifier of Clustered Objects (AMICO) to detect and characterize groups and clusters of galaxies down to S/N=2.5 in the redshift range 0.05<z<0.8. We detect 80, 30 and 11 systems with signal-to-noise ratio larger than 2.5, 3.0 and 3.5, respectively, down to ~10^13^M_{sun}_/h. We derive mass-proxy scaling relations based on Chandra and XMM-Newton X-ray data for the signal amplitude returned by AMICO, the intrinsic richness and a new proxy that incorporates the galaxies' stellar masses. The latter proxy is made possible thanks to the J-PAS filters and shows a smaller scatter with respect to the richness. We fully characterize the sample and use AMICO to derive a probabilistic membership association of galaxies to the detected groups that we test against spectroscopy. We further show how the narrow band filters of J-PAS provide a gain of up to 100% in signal-to-noise ratio in detection and an uncertainty on the redshift of clusters of only {sigma}_z_=0.0037(1+z) placing J-PAS in between broadband photometric and spectroscopic surveys. The performances of AMICO and J-PAS with respect to mass sensitivity, mass-proxies quality.2023A&A...678A.145Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/678/A145CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/645/A87 : Star-galaxy classification feature importance (Baqui+, 2021)J/A+A/672/A137 : AGN and host galaxy co-evolution (Lopez+, 2023)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/678/A145https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/678/A145http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/678/A145https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/678/A145https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/678/A145http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/678/A145GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/678/A145/clusters (Galaxy clusters detections)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/678/A145/clusters?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/678/A145/clusters?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/678/A145/clusters?GETtext/xml+votable180.050000true213.344752.16330.005555555555555556Cone search capability for table J/A+A/678/A145/members (Cluster members)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/678/A145/members?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/678/A145/members?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/678/A145/members?GETtext/xml+votable180.050000true213.531351.99332390.005555555555555556Cone search capability for table J/A+A/678/A145/bggs (Clusters BGGs)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/678/A145/bggs?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/678/A145/bggs?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/678/A145/bggs?GETtext/xml+votable180.050000true213.6254351.937870.0055555555555555566/10741 10743 11424-11426 11428https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/678/A145?format=asciiX-rayOpticaldefaultJ/A+A/678/A145/clustersGalaxy clusters detectionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSurvey[JPm] Survey name (SURVEY)meta.idcharNameObject name (JHHMMSS.ss+DDMMSS) (NAME)meta.id;meta.maincharCluster[1/80] Unique identification number of the cluster (ID)meta.idintAMICO[1/1144] AMICO identification number (IDAMICO)meta.idintRAJ2000Right Ascension (J2000) (RA)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) (DEC)degpos.eq.dec;meta.mainzRedshift (Z)src.redshiftfloate_z1-sigma uncertainty of Z (ZERR)stat.error;src.redshiftfloatzProbRedshift based on AMICO membership (ZPROB)src.redshift;pos.heliocentricfloate_zProb1-sigma uncertainty of ZPROB (ZPROB_ERR)stat.errorfloatzsp? Spectroscopic redshift (when available) (ZSPEC)src.redshiftdoublenullableNSpecNumber of members with spectroscopic redshift (NSPEC)meta.numberintSNSignal-to-noise ratio of AMP; noise = background + cluster (SN)stat.snr;instr.backgroundfloatMaskFracFraction of the cluster inaccessible because of mask (MASKFRAC)meta.numberfloatRmedianMedian separation of galaxies with P>50% (RMEDIAN)degpos.angDistance;stat.medianfloatR50Radius at which {int}_0_^r^P(r)/{int}_0_^inf^P(r)=0.5 (R50)degphys.angSizefloatRichMedian separation of galaxies with P>50% (RICH)pos.angDistance;stat.medianfloatAmpSignal amplitude (AMP)stat.snr;src.var.amplitudefloate_Amp1 sigma error on Amp (AMPERR)stat.errorfloatLambdaRichness based on memberships (LAMBDA)src.class.richnessfloate_Lambda1 sigma error on Lambda (LAMBDAERR)stat.errorfloatLambdaStarRichness based on membership and m_r_<m_star_+1.5 and r<r_vir_ (LAMBDASTAR)src.class.richnessfloate_LambdaStar1 sigma error on LambdaStar (LAMBDASTARERR)stat.errorfloatLambdaMstarTotal stellar mass based on membership and log10(M_star_)>9.5 (LAMBDAMSTAR)1e+12solMassphys.massfloate_LambdaMstar1-sigma uncertainty on LambdaMstar (LAMBDAMSTARERR)1e+12solMassstat.errorfloatMassAXMass based on the amplitude and the X-ray scaling relation (MASSAX)1e+13solMassphys.massfloate_MassAX1-sigma uncertainty of MassAX (MASSAXERR)1e+13solMassstat.errorfloatMassX? Mass based on X-rays (MASSX)1e+13solMassphys.massfloatnullablee_MassX? 1-sigma uncertainty on MassX (MASSXERR)1e+13solMassstat.errorfloatnullableLX? X-ray luminosity (in 10^42^erg/s) (LX)1e+35Wphys.luminosity;em.X-rayfloatnullablee_LX? 1-sigma uncertainty on LX (in 10^42^erg/s) (LXERR)1e+35Wstat.errorfloatnullableSNX? Signal-to-noise ratio of the X-ray flux (SNX)stat.snrfloatnullableIDBCG1Identification number of the BGG galaxy, first choice (IDBCG1)meta.idintIDBCG2Identification number of the BGG galaxy, second choice (IDBCG2)meta.idintJ/A+A/678/A145/membersCluster membersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxy[83/20866] Galaxy identification number (ID)meta.id;meta.mainintRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (DEC)degpos.eq.dec;meta.mainindexedXpixSky position in the AMICO amplitude maps fits file (Xpix)pixpos.cartesian.x;meta.fitsdoubleYpixSky position in the AMICO amplitude maps fits file (Ypix)pixsrc.var.amplitude;meta.fitsdoubler'magr' magnitude (RMAG)magphot.mag;em.opt.RdoublePField[0/1] Probability to belong to the field (FIELDPROB)stat.fit.goodnessdoubleAssoc[1/1144] Identification number of the AMICO associated cluster (ASSOCIT)meta.numberintPAssoc[0/1] Probabilistic membership association of galaxies to clusters (ASSOCPROB)meta.code.memberdoubleTileIdentification number of the tile (optical image) (TILEID)obs.fieldintJ/A+A/678/A145/bggsClusters BGGsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxy[292/20812] Galaxy identification number (GALID)meta.id;meta.mainintRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) (DEC)degpos.eq.dec;meta.mainXpixSky position in the AMICO amplitude maps fits file (Xpix)pixpos.cartesian.x;meta.fitsdoubleYpixSky position in the AMICO amplitude maps fits file (Ypix)pixsrc.var.amplitude;meta.fitsdoubler'magr' magnitude (RMAG)magphot.mag;em.opt.RdoublePField[0/1] Probability to belong to the field (FIELDPROB)stat.fit.goodnessdoubleNassocNumber of associated detections (ASSOCNUMBER)meta.numberintAssoc[1/1144] Identification number of the AMICO associated cluster (ASSOCID)meta.numberintPAssoc[0/1] Probabilistic membership association of galaxies to clusters (ASSOCPROB)meta.code.memberdoubleRank[1/2] Rank of the galaxy: 1 = brightest, 2 = second brightest (CDRANK)meta.codeint