J/A+A/691/A300ivo://CDS.VizieR/J/A+A/691/A300doi:10.26093/cds/vizier.36910300CDSXu W.Jiang L.Li R.Luo B.Brandt W.N.Zhang C.Erben T.2025-02-13T20:01:24Z2024-11-20T08:03:28ZCDS support team

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

cds-question@unistra.frgalaxy-clustersx-ray-sourcesTo explain the well-known tension between cosmological parameter constraints obtained from the primary cosmic microwave background (CMB) and those drawn from X-ray-selected galaxy cluster samples identified with early data, we propose a possible explanation for the incompleteness of detected clusters being higher than estimated. Specifically, we suggest that certain types of galaxy groups or clusters may have been overlooked in previous works. We aim to search for galaxy groups and clusters with especially extended surface brightness distributions by creating a new X-ray-selected catalog of extended galaxy clusters from the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) data, based on a dedicated source detection and characterization algorithm optimized for extended sources. Our state-of-the-art algorithm is composed of wavelet filtering, source detection, and characterization. We carried out a visual inspection of the optical image, and spatial distribution of galaxies within the same redshift layer to confirm the existence of clusters and estimated the cluster redshift with the spectroscopic and photometric redshifts of galaxies. The growth curve analysis was used to characterize the detections. We present a catalog of extended X-ray galaxy clusters detected from the XMM-SERVS data. The XMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog features 141 cluster candidates. Specifically, there are 53 clusters previously identified as clusters with intracluster medium (ICM) emission (class 3); 40 that were previously known as optical or infrared (IR) clusters, but detected as X-ray clusters for the first time (class 2); and 48 identified as clusters for the first time (class 1). Compared with the class 3 sample, the "class 1 + class 2" sample is systematically fainter and exhibits a flatter surface brightness profile. Specifically, the median flux in [0.5-2.0]keV band for `class 1 + class 2" and class 3 sample is 1.288*10^-14^erg/s/cm^2^ and 1.887*10^-14^erg/s/cm^2^, respectively. The median values of beta (i.e., the slope of the cluster surface brightness profile) are 0.506 and 0.573 for the "class 1 + class 2" and class 3 samples, respectively.2024A&A...691A.300Xhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/691/A300CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/478/2132 : XMM-SERVS survey: XMM-LSS field new XMM-Newton point-sourcesJ/ApJS/256/21 : XMM-SERVS survey: X-ray sources for W-CDF-S + ELAIS-S1https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/691/A300https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/691/A300http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/691/A300https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/691/A300https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/691/A300http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/691/A300GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/691/A300/xvxgc (XMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog (table B1))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/691/A300/xvxgc?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/691/A300/xvxgc?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/691/A300/xvxgc?GETtext/xml+votable180.050000true8.618-43.3160.0055555555555555565/4422 6/17677 17681-17683 17686 17692 17712-17713 35382 35388 35390 35473 35476 35933-35935 35953 35956-35957 36106https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/691/A300?format=asciiX-raydefaultJ/A+A/691/A300/xvxgcXMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog (table B1)r_zSource of redshiftmeta.ref;pos.framecharExtMLExtension likelihoodstat.likelihooddoubleExtentExtentarcminphys.angSizefloatRsigSignificant radiusarcminphys.angSizefloatCRRsigSum of count rate within Rsigct/sphot.count;em.X-rayfloate_CRRsig1sigma error of CRRsigct/sstat.errorfloatR500R500 in the unit of arcminarcminphys.angSizefloatR500MpcR500 in the unit of MpcMpcphys.size.radiusfloate_R500Mpc1sigma error of R500[Mpc]Mpcstat.errorfloatCRR500Total count rate within R500ct/sphot.count;em.X-rayfloate_CRR5001sigma error of CR500ct/sstat.errorfloatF500F500 at [0.5-2.0]keV (in erg/s/cm^2^)mW.m**-2phot.flux;em.X-raydoublee_F5001sigma error of F500 (in erg/s/cm^2^)mW.m**-2stat.errordoubleL500L500 at rest-frame [0.5-2.0]keV (in erg/s)1e-07Wphys.luminosity;em.X-raydoublee_L5001sigma error of L500 (in erg/s)1e-07Wstat.errordoubleTxTemperature of ICMkeVphys.temperaturefloate_Tx1sigma error of TxkeVstat.errorfloatM500Mass within R500solMassphys.massdoublee_M5001sigma error of M500solMassstat.errordoubleBetaBeta valuemeta.crypticfloate_BetaLower 1sigma error of Betastat.errorfloatE_BetaUpper 1sigma error of Betastat.error;stat.maxfloatRcCore radiusarcminphys.angSizefloate_RcLower 1sigma error of Rcarcminstat.errorfloatE_RcUpper 1sigma error of Rcarcminstat.error;stat.maxfloatCommentComment on this sourcemeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameDesignation (es_NNN)meta.id;meta.maincharRAJ2000Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainClassClassmeta.code.classintNmemNumber of member galaxiesmeta.numberintzRedshiftsrc.redshiftfloate_z1sigma error of redshiftstat.error;src.redshiftfloat