J/ApJ/890/148ivo://CDS.VizieR/J/ApJ/890/148doi:10.26093/cds/vizier.18900148CDSUmetsu K.Sereno M.Lieu M.Miyatake H.Medezinski E.Nishizawa A.J.,Giles P.Gastaldello F.McCarthy I.G.Kilbinger M.Birkinshaw M.,Ettori S.Okabe N.Chiu I.-N.Coupon J.Eckert D.Fujita Y.,Higuchi Y.Koulouridis E.Maughan B.Miyazaki S.Oguri M.Pacaud F.,Pierre M.Rapetti D.Smith G.P.2021-09-29T12:17:21Z2021-08-18T16:11:11ZCDS support team

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

cds-question@unistra.frgalaxy-clustersx-ray-sourcesredshiftedvisible-astronomygravitational-lensingWe present a weak-lensing analysis of X-ray galaxy groups and clusters selected from the XMM-XXL survey using the first-year data from the Hyper Suprime-Cam (HSC) Subaru Strategic Program. Our joint weak-lensing and X-ray analysis focuses on 136 spectroscopically confirmed X-ray-selected systems at 0.031<=z<=1.033 detected in the 25deg^2^ XXL-N region, which largely overlaps with the HSC-XMM field. With high-quality HSC weak-lensing data, we characterize the mass distributions of individual clusters and establish the concentration-mass (c-M) relation for the XXL sample, by accounting for selection bias and statistical effects and marginalizing over the remaining mass calibration uncertainty. We find the mass-trend parameter of the c-M relation to be {beta}=-0.07+/-0.28 and the normalization to be c_200_=4.8+/-1.0(stat)+/-0.8(syst) at M_200_=10^14^h^-1^M_{sun}_ and z=0.3. We find no statistical evidence for redshift evolution. Our weak-lensing results are in excellent agreement with dark-matter-only c-M relations calibrated for recent {Lambda}CDM cosmologies. The level of intrinsic scatter in c200 is constrained as {sigma}(lnc_200_)<24% (99.7% CL), which is smaller than predicted for the full population of {Lambda}CDM halos. This is likely caused in part by the X-ray selection bias in terms of the cool-core or relaxation state. We determine the temperature-mass (T_X_-M_500_) relation for a subset of 105 XXL clusters that have both measured HSC lensing masses and X-ray temperatures. The resulting TX-M500 relation is consistent with the self-similar prediction. Our TX-M500 relation agrees with the XXL DR1 results at group scales but has a slightly steeper mass trend, implying a smaller mass scale in the cluster regime. The overall offset in the TX-M500 relation is at the ~1.5{sigma} level, corresponding to a mean mass offset of 34%+/-20%. We also provide bias-corrected, weak-lensing-calibrated M200 and M500 mass estimates of individual XXL clusters based on their measured X-ray temperatures.2020ApJ...890..148Uhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/890/148CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIX/49 : XXL Survey: First results (Pierre+, 2016)IX/52 : XXL Survey. DR2 (Chiappetti+, 2018)J/ApJ/690/1236 : COSMOS photometric redshift catalog (Ilbert+, 2009)J/ApJS/199/25 : CLASH sources for MACS1149.6+2223 (Postman+, 2012)J/MNRAS/444/147 : Richness of galaxy clusters (Oguri, 2014)J/ApJS/216/27 : Galaxy clusters in the SPT-SZ survey (Bleem+, 2015)J/A+A/581/A41 : OmegaWINGS BV phot. of galaxy clusters (Gullieuszik+, 2015)J/MNRAS/450/3675 : CoMaLit. IV. Sigma Catalogue (Sereno+, 2015)J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)J/ApJS/224/1 : redMaPPer cluster catalog from DES data (Rykoff+, 2016)J/A+A/607/A81 : Properties of the sample of clusters (Biviano+, 2017)J/MNRAS/468/1917 : Concentration parameter of galaxy clusters (Rossetti+, 2017)J/MNRAS/468/3322 : CoMaLit. V. Mass forecasting with proxies (Sereno+, 2017)J/PASJ/70/S20 : HSC Wide S16A cluster catalog (Oguri+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/890/148https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/890/148http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/890/148https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/890/148https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/890/148http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/890/148GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/890/148/table2 (Cluster properties and weak-lensing measurements)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/890/148/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/890/148/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/890/148/table2?GETtext/xml+votable180.050000true36.384-3.920.0055555555555555565/4421-4423 4425 6/17675 17677-17679 17681-17683 17697-17699 17705 17712-17713 17715-17717https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/890/148?format=asciiX-rayOpticaldefaultJ/ApJ/890/148/table2Cluster properties and weak-lensing measurementsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintXLSSC[2/202] Identifier (1)meta.id;meta.mainintRAJ2000[30.42/38.51] X-ray cluster right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[-6.21/-2.66] X-ray cluster declination (J2000)degpos.eq.dec;meta.mainz[0.03/1.04] Redshiftsrc.redshiftfloatCl[1/2] Object class (2)meta.codeintT300kpc[0.63/6.03]? X-ray temperature, T_300kpc_keVphys.temperaturefloatnullablee_T300kpc[0.03/1.05]? T300kpc downwards uncertaintykeVstat.errorfloatnullableE_T300kpc[0.04/1.14]? T300kpc upwards uncertaintykeVstat.error;stat.maxfloatnullablec200[2/9.6] Concentration parameter c_200_=r_200_/r_s_ (section 4.1) (3)stat.paramfloate_c200[1.2/5.6] C200 uncertaintystat.errorfloatc200Med[1.9/9.3] Median value of c200stat.medianfloatM200[0.07/9.64] Mass enclosed within a sphere of radius r_200_ (3)1e+14solMassphys.massfloate_M200[0.08/7.94] M200 uncertainty1e+14solMassstat.errorfloatM200Med[0.07/9.45] Median value of M2001e+14solMassphys.mass;stat.medianfloatM500[0.05/5.59] Mass, M_500_ (3)1e+14solMassphys.massfloate_M500[0.05/5.5] M500 uncertainty1e+14solMassstat.errorfloatM500Med[0.05/5.53] Median value of M5001e+14solMassphys.mass;stat.medianfloatM200MT[0.2/6.8]? Bias-corrected, weak-lensing-calibrated mass estimates, M_200,MT_ (4)1e+14solMassphys.massfloatnullablee_M200MT[0.1/2.2]? M200MT downwards uncertainty1e+14solMassstat.errorfloatnullableE_M200MT[0.19/3.4]? M200MT upwards uncertainty1e+14solMassstat.error;stat.maxfloatnullableM500MT[0.16/4.72]? Bias-corrected, weak-lensing-calibrated mass estimates, M_500,MT_ (4)1e+14solMassphys.massfloatnullablee_M500MT[0.08/1.35]? M500MT downwards uncertainty1e+14solMassstat.errorfloatnullableE_M500MT[0.14/1.92]? M500MT upwards uncertainty1e+14solMassstat.error;stat.maxfloatnullableS/N[-2.1/6] Signal-to-noise ratio based on the linear estimator (Equation (13))stat.snrfloatSNRq[0.8/9.1] Signal-to-noise ratio based on the quadratic estimator (Equation (15))stat.snrfloatR18Display data from XXL DR2 cat. (IX/52), Paper XXVIIImeta.ref.urlintnullableSimbadSimbad column added by the CDSmeta.ref.urlchar