J/ApJ/934/129ivo://CDS.VizieR/J/ApJ/934/129doi:10.26093/cds/vizier.19340129CDSSalvati L.Saro A.Bocquet S.Costanzi M.Ansarinejad B.Benson B.A.,Bleem L.E.Calzadilla M.S.Carlstrom J.E.Chang C.L.Chown R.,Crites A.T.de Haan T.Dobbs M.A.Everett W.B.Floyd B.Grandis S.,George E.M.Halverson N.W.Holder G.P.Holzapfel W.L.Hrubes J.D.,Lee A.T.Luong-Van D.McDonald M.McMahon J.J.Meyer S.S.Millea M.,Mocanu L.M.Mohr J.J.Natoli T.Omori Y.Padin S.Pryke C.,Reichardt C.L.Ruhl J.E.Ruppin F.Schaffer K.K.Schrabback T.,Shirokoff E.Staniszewski Z.Stark A.A.Vieira J.D.Williamson R.2024-11-06T20:26:15Z2024-08-16T08:56:29ZCDS support team

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

cds-question@unistra.frgalaxy-clustersredshiftedmillimeter-astronomysubmillimeter-astronomysurveysWe provide the first combined cosmological analysis of the South Pole Telescope (SPT) and Planck cluster catalogs. The aim is to provide an independent calibration for Planck scaling relations, exploiting the cosmological constraining power of the SPT-SZ cluster catalog and its dedicated weak lensing (WL) and X-ray follow-up observations. We build a new version of the Planck cluster likelihood. In the {nu}{Lambda}CDM scenario, focusing on the mass slope and mass bias of Planck scaling relations, we find {alpha}_SZ_=1.49_-0.10_^+0.07^ and (1-b)_SZ_=0.69_-0.14_^+0.07^, respectively. The results for the mass slope show a ~4{sigma} departure from the self-similar evolution, {alpha}_SZ_~1.8. This shift is mainly driven by the matter density value preferred by SPT data, {Omega}_m_=0.30+/-0.03, lower than the one obtained by Planck data alone, {Omega}_m_=0.37_-0.06_^+0.02^. The mass bias constraints are consistent both with outcomes of hydrodynamical simulations and external WL calibrations, (1-b)~0.8, and with results required by the Planck cosmic microwave background cosmology, (1-b)~0.6. From this analysis, we obtain a new catalog of Planck cluster masses M_500_. We estimate the ratio between the published Planck MSZ masses and our derived masses M_500_, as a "measured mass bias", (1-b)_M_. We analyze the mass, redshift, and detection noise dependence of (1-b)_M_, finding an increasing trend toward high redshift and low mass. These results mimic the effect of departure from self-similarity in cluster evolution, showing different dependencies for the low-mass, high-mass, low-z, and high-z regimes.2022ApJ...934..129Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/934/129CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/774/23 : Chandra observations of SPT-SZ clusters (McDonald+, 2013)J/ApJ/792/45 : SPT-SZ survey galaxy clusters opt. spectroscopy (Ruel+, 2014)J/ApJS/216/27 : Galaxy clusters discovered in the SPT-SZ survey (Bleem+, 2015)J/MNRAS/449/835 : Clustering of SDSS DR7 main galaxy sample. I. (Ross+, 2015)J/MNRAS/450/3675 : CoMaLit. IV. Sigma Catalogue (Sereno+, 2015)J/A+A/580/A95 : Planck/AMI Sunyaev-Zel'dovich measurements (Perrott+, 2015)J/A+A/594/A27 : Planck Sunyaev-Zeldovich sources (PSZ2) (Planck+, 2016)J/ApJS/227/3 : Full sp. data release of the SPT-GMOS (Bayliss+, 2016)J/PAZh/43/559 : Planck galaxy cluster catalogue extension (Burenin, 2017)J/AJ/153/220 : NORAS II. I. First results (Bohringer+, 2017)J/ApJ/853/36 : Sp. obs. of 20 Planck gal. cluster cand. (Amodeo+, 2018)J/ApJ/878/55 : SPT-SZ clusters with optical & X-ray data (Bocquet+, 2019)J/MNRAS/488/739 : MARD-Y3 catalog (Klein+, 2019)J/A+A/631/A148 : PSZ2 cluster candidates. II. (Aguado-Barahona+, 2019)J/ApJS/247/25 : The SPTpol Extended Cluster Survey (Bleem+, 2020)J/ApJ/892/102 : XMM X-ray data of Planck ESZ galaxy clusters (Lovisari+, 2020)J/ApJ/900/55 : The SPT-SZ catalog at 95, 150, and 220GHz (Everett+, 2020)J/A+A/647/A106 : PSZSPT, joint Planck & SPT-SZ cluster cat. (Melin+, 2021)J/A+A/655/A115 : PSZ1 galaxy clusters {sigma} and Mdyn (Ferragamo+, 2021)J/ApJS/253/3 : Sunyaev-Zel'dovich galaxy clusters with ACT (Hilton+, 2021)J/A+A/661/A2 : Galaxy clusters and groups in eFEDS (Liu+, 2022)J/other/RNAAS/7.51 : Brightest galaxies in Planck clusters (Smith+, 2023)J/MNRAS/531/1998 : ComPACT, ACT+Planck gal. clusters (Voskresenksaia+, 2024)http://pla.esac.esa.int/ : Planck Legacy Archivehttp://pole.uchicago.edu/public/data/sptplanck_cluster/ : SPT-SZ and Planckhttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/934/129https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/934/129http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/934/129https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/934/129https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/934/129http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/934/129GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/934/129/table5 (the New Planck Cluster Catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/934/129/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/934/129/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/934/129/table5?GETtext/xml+votable180.050000true229.19051-1.017220.0055555555555555566/136 708 2388 2432 2488 4206 4394 4406 4816 4946 4965 5099-5100 5327 5346 5524 5536 5597 5701 5931 5985 6011 6019 6088 6337 6383 6441 6474 6609 6772 6873 7026 7115 7206 7221 7239 7242 7387 7448 7513 7579 7649 7695 7768 7928 8033 8066 8139 8220 8271 8338 8507 8520 8648 8745 8875 8947 8963 9036 9050 9072 9124 9168 9354 9366 9468 9476 9496 9506 9508 9588 9593 9664 9764 9776 9787 9997 10271 10311-10312 10318 10379 10397 10401 10416 10526-10527 10664 10716 10822 10959 10998 11041-11042 11063 11080 11216 11222 11253 11264 11279 11419 11436 11442-11443 11463 11467 11591 11613 11626 11672 11795 11807 11809 11846 11912 11920 12072 12121 12168 12184 12298 12504 12560 12642 12653 12736 13314 13387 14879 15066 15112 15129 15233 15286 15296 15345 15351 15903 15979 16024 16030 16032 16072 16075 16411 16434 16486 16492 16510 16524 16543 16609 16642 16661 16702 16713 16765 16782 16787 16801 16806 16982 17044 17084 17141 17237 17247 17300 17357 17387 17438 17457 17499 17504 17518 17712 17741 17744 17936 18016 18064 18110 18290 18475 18534 18566 18584 18683 18746 18800 18894 19009 19055 19089 19101 19124 19269 19451 19461 19542 19656 19678 19848 19858 19935 19993 20029 20128 20247 20302 20335 20355 20392 20427 20481 20507 20520 20536 20579 20624 20643 20735 20874 21073 21133 21156 21766 21894 21934 21971 22012 22330 22373 22467 22490-22491 22577 22607 22661 22792 22915 22972 24622 24735 24822 24943 25135 25166 25188 25331 25391 25451 25542 25675 25852 26037 26135 26189 26208 26377 26668 26770 26785 27075 27087 27136 27327 27428 27574 27660 27740 27742 27765 27966 28022 28174 28181 28202 28251 28271-28272 28372 28429-28430 28448 28490 28556 28622 28631 31396 31495 31537 32362 32379 32500 32503 32693 32766 32798 32894-32895 32960 33030 33034 33152 33180 33235 33289 33321 33474 33509 33586 33614 33628 33649 33692 33718 33796 33810 33827 33871 33891 33945 34049 34087 34159 34174 34181 34186 34229 34324 34443 34461 34580 34726 34805 34910 35015 35043 35055 35147 35171 35310 35388 35417 35758 35808 35950 36017 36089 36150 36434 37095 37378 38246 38704 38822 38858 38944 38973 39043 39067-39068 39077 39079 39443 39462 39552 39608 40351 40564 40809 41077 41081 43358 43428 43627 43637 43706 43837-43838 43849 43939 43948 43977 44008 44017 44041 44802 44817 45044 45076 45177 45421 45433 45435 45506 45543 45546 45562 45741 45893 45965-45966 45981 45984 46237 46301 46389 46424 46444 46474 46540 46571 46660 46687 46763 46855 46889 46892 46952 47139 47168 47188 47225 47314 47463 47573 47919 48076 48133 48258 48375 48489 48735 48966https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/934/129?format=asciiMillimeterdefaultJ/ApJ/934/129/table5the New Planck Cluster Cataloge_M500freeLower 68% confidence limit of M500free (M500_free_low)stat.errordoubleM500fix[7.2e+13/1.6e+15] Mass, M_500_, for fixed values of cosmological and scaling relation parameters reported in Table 7; in 10^14^M_{sun}_h^-1^ units (M500_fixed_bf)phys.mass;meta.modelleddoubleE_M500fixUpper 68% confidence limit of M500fix (M500_fixed_up)stat.error;stat.max;phys.massdoublee_M500fixLower 68% confidence limit of M500fix (M500_fixed_low)stat.error;stat.min;phys.massdoubleSimbadSimbad column added by the CDSmeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlcharM500free[4.7e+13/1.6e+15] Mass, M_500_, obtained by marginalizing over the cosmological and scaling relation parameters from our SPTcl+PvSPLIT analysis in 10^14^M_{sun}_h^-1^ units (M500_free_bf)phys.mass;meta.modelleddoubleE_M500freeUpper 68% confidence limit of M500free (M500_free_up)stat.error;stat.maxdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPSZ2Name (GLLL.ll+bb.bb) (name) (1)meta.id;meta.maincharRAJ2000Right ascension (J2000) (ra) (1)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) (dec) (1)degpos.eq.dec;meta.mainz[0.01/1] Redshift (z) (1)src.redshiftdoubleSNR[6/49] Signal-to-noise ratio of the detection (q) (1)stat.snrdouble