J/ApJ/878/55ivo://CDS.VizieR/J/ApJ/878/55doi:10.26093/cds/vizier.18780055CDSBocquet S.Dietrich J.P.Schrabback T.Bleem L.E.Klein M.Allen S.W.,Applegate D.E.Ashby M.L.N.Bautz M.Bayliss M.Benson B.A.Brodwin M.,Bulbul E.Canning R.E.A.Capasso R.Carlstrom J.E.Chang C.L.Chiu I.,Cho H.-M.Clocchiatti A.Crawford T.M.Crites A.T.de Haan T.Desai S.,Dobbs M.A.Foley R.J.Forman W.R.Garmire G.P.George E.M.,Gladders M.D.Gonzalez A.H.Grandis S.Gupta N.Halverson N.W.,Hlavacek-Larrondo J.Hoekstra H.Holder G.P.Holzapfel W.L.Hou Z.,Hrubes J.D.Huang N.Jones C.Khullar G.Knox L.Kraft R.Lee A.T.,von der Linden A.Luong-Van D.Mantz A.Marrone D.P.McDonald M.,McMahon J.J.Meyer S.S.Mocanu L.M.Mohr J.J.Morris R.G.Padin S.,Patil S.Pryke C.Rapetti D.Reichardt C.L.Rest A.Ruhl J.E.,Saliwanchik B.R.Saro A.Sayre J.T.Schaffer K.K.Shirokoff E.,Stalder B.Stanford S.A.Staniszewski Z.Stark A.A.Story K.T.,Strazzullo V.Stubbs C.W.Vanderlinde K.Vieira J.D.Vikhlinin A.,Williamson R.Zenteno A.2021-09-16T10:45:03Z2020-12-21T11:44:24ZCDS support team

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

cds-question@unistra.frgalaxy-clustersredshiftedvisible-astronomygravitational-lensingx-ray-sourcessurveysWe derive cosmological constraints using a galaxy cluster sample selected from the 2500deg^2^ SPT-SZ survey. The sample spans the redshift range 0.25<z<1.75 and contains 343 clusters with SZ detection significance {xi}>5. The sample is supplemented with optical weak gravitational lensing measurements of 32 clusters with 0.29<z<1.13 (from Magellan and Hubble Space Telescope) and X-ray measurements of 89 clusters with 0.25<z<1.75 (from Chandra). We rely on minimal modeling assumptions: (i) weak lensing provides an accurate means of measuring halo masses, (ii) the mean SZ and X-ray observables are related to the true halo mass through power-law relations in mass and dimensionless Hubble parameter E(z) with a priori unknown parameters, and (iii) there is (correlated, lognormal) intrinsic scatter and measurement noise relating these observables to their mean relations. We simultaneously fit for these astrophysical modeling parameters and for cosmology. Assuming a flat {nu}{Lambda}CDM model, in which the sum of neutrino masses is a free parameter, we measure {Omega}_m_=0.276+/-0.047, {sigma}_8_=0.781+/-0.037, and {sigma}_8_({Omega}_m_/0.3)^0.2^=0.766+/-0.025. The redshift evolutions of the X-ray Y_X_-mass and M_gas_-mass relations are both consistent with self-similar evolution to within 1{sigma}. The mass slope of the Y_X_-mass relation shows a 2.3{sigma} deviation from self-similarity. Similarly, the mass slope of the M_gas_-mass relation is steeper than self-similarity at the 2.5{sigma} level. In a {nu}wCDM cosmology, we measure the dark energy equation-of-state parameter w=-1.55+/-0.41 from the cluster data. We perform a measurement of the growth of structure since redshift z~1.7 and find no evidence for tension with the prediction from general relativity. This is the first analysis of the SPT cluster sample that uses direct weak-lensing mass calibration and is a step toward using the much larger weak-lensing data set from DES. We provide updated redshift and mass estimates for the SPT sample.2019ApJ...878...55Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/878/55CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/hst : HST Archived Exposures Catalog (STScI, 2007)B/chandra : The Chandra Archive Log (CXC, 1999-2014)J/ApJ/694/992 : SED of cluster radio galaxies (Lin+, 2009)J/ApJ/761/22 : NIR galaxy cluster candidates in the SPT survey (Song+, 2012)J/ApJ/774/23 : Chandra observations of SPT-SZ clusters (McDonald+, 2013)J/ApJ/763/127 : Galaxy clusters discovered in SPT survey (Reichardt+, 2013)J/ApJ/774/23 : Chandra observations of SPT-SZ clusters (McDonald+, 2013)J/ApJ/779/61 : SPT-SZ survey at 95, 150 & 220GHz (Mocanu+, 2013)J/ApJ/792/45 : SPT-SZ survey galaxy clusters opt. spectroscopy (Ruel+, 2014)J/ApJS/216/27 : Galaxy clusters discovered in SPT-SZ survey (Bleem+, 2015)J/MNRAS/449/835 : Clustering of SDSS DR7 main galaxy sample. I. (Ross+, 2015)J/ApJS/227/3 : Full spectroscopic release of the SPT-GMOS (Bayliss+, 2016)J/ApJS/224/1 : redMaPPer cluster catalog from DES data (Rykoff+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/878/55https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/878/55http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/878/55https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/878/55https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/878/55http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/878/55GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/878/55/table5 (Galaxy cluster candidates with {xi}>4.5 in the 2500 square-degree South Pole Telescope Sunyaev Zel'dovich (SPT-SZ) survey)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/878/55/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/878/55/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/878/55/table5?GETtext/xml+votable180.050000true0.0663-43.94940.0055555555555555565/8552 8576 11471 6/16385 20480 33117 33141 33149 33180 33203 33212-33213 33223-33225 33234-33236 33240-33241 33251-33252 33261-33262 33270 33273-33274 33277 33391 33395 33400 33464 33471 33474 33487 33497 33502 33509 33514-33517 33520 33527 33529 33531 33534 33537 33540 33543 33548 33553-33554 33564 33571 33573 33578 33580 33586 33593-33594 33598 33603-33604 33610 33614 33616 33618-33619 33625 33632 33638 33642 33644 33649 33656-33657 33660 33662 33668 33674 33696 33700 33706 33709 33712-33713 33718 33725 33728 33735 33741 33743 33746 33748 33754-33755 33758 33762-33765 33768-33769 33773 33779 33783 33796 33799 33810 33814 33816-33818 33820 33824 33826-33828 33832-33833 33846 33850-33851 33856 33863 33865 33871 33877-33878 33894 33897 33905 33910-33912 33921 33932 33938 33945 33948 33950 33956-33957 33960 33969-33971 33978 33982 33989-33990 33993 33996-33997 33999 34001-34003 34007-34009 34014 34026 34030 34032 34035 34043 34049 34053 34055 34059-34060 34063 34066-34067 34074 34076 34082-34083 34087 34103 34111 34119 34125 34130 34133 34139 34142 34150 34156 34179 34181-34182 34198 34202 34215 34227 34309 34316 34323-34324 34326 34330 34333 34335-34336 34338 34345 34348 34350 34353 34355 34357 34362 34368-34369 34372 34375 34377 34379 34384 34411-34412 34433 34444 34459-34461 34465 34473 34477 34498 34504 34821-34822 34836 34839 34845 34848 34857 34876 34881 34888 34891 34893 34899 34909-34910 34915 34921-34922 34927 34932 34935 34943 34953-34954 34962 34972 34974 34978 34980 34985-34987 34993 35000-35001 35003 35007-35008 35018 35020 35032 35043-35044 35052 35058 35065 35070 35086 35090 35097 35107-35108 35114 35121 35124-35125 35129-35130 35133 35135 35147 35156-35157 35162 35168 35171 35176 35201 35203 35206 35209 35215 35219 35222 35238 35252 35335-35337 35342-35343 35346 35348 35359 35364 35370 35376 35382 35387-35388 35396-35397 35399-35400 35405 35407 35417 35419 35424 35436 35441 35457 35460 35469 35482-35483 35490 35493 35495 35498 35501 35520 38918 38928 38936 38955 38960-38961 38966 38973 38975 39043-39044 39051 39067-39069 39076 39097 39100 39102 39106 39431-39432 39441 39443 39449 39452-39453 39463 39467 39469 39472 39477 39481-39483 39486 39491 39498-39499 39529 39531 39552 39561 39564 39570 39572 39577 39586 39588 39594 45421 45424 45433 45435 45484-45485 45490-45491 45497-45500 45506 45522 45526 45533 45536 45539 45543-45544 45546 45554-45555 45563 45662 45686 45692 45791 45815 45830 45835 45839 45841 45844 45850 45860 45862 45867 45873 45876 45893-45894 45904 45907 45909 45911-45912 45918 45921 45932 45934 45946 45949 45957 45959 45962-45966 45968 45973 45979 45984 45987 45995 45997 46001 46005 46009 46021 46028 46039 46045-46046 46058 46067 46069 46071 46078 46083 46097 46100-46101 46108-46110 46120 46127 46131 46139 46142-46143 46145 46149 46153 46160-46161 46166 46169-46170 46179 46182 46196 46202 46207 46229 46235 46240 46243 46257-46258 46268 46272 46276 46290 46296-46297 46301 46311-46312 46321 46323 46327 46332 46334 46338 46340-46341 46345 46353 46364 46368 46380 46382 46387-46389 46394 46402 46417 46420-46421 46424 46436 46444 46448 46470 46474 46484-46485 46487 46491 46494 46499 46511 46516 46595 46599 46610 46612 46614 46616-46617 46628-46629 46632 46636 46641-46642 46652 46656 46660 46689 46693 46695 46704 46738-46739 46748 46750 46752 46768 46770 47364 47378 47382 47384 47390 47414 47417 47430 47434 47438 47446 47448 47450 47455-47456 47459 47463 47509 48130https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/878/55?format=asciiX-rayOpticaldefaultJ/ApJ/878/55/table5Galaxy cluster candidates with {xi}>4.5 in the 2500 square-degree South Pole Telescope Sunyaev Zel'dovich (SPT-SZ) surveyl_zLimit flag on z (2)meta.code.error;src.redshiftcharn_zNote on z (3)meta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSPT-CLSPT-CL identifier (JHHMM+DDMM)meta.id;meta.maincharn_SPT-CLNote on SPT-CL (1)meta.notecharRAJ2000[0/360] Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[-65.32/-39.8] Declination (J2000)degpos.eq.dec;meta.mainxi[4.5/42.4] Highest detection significance in the filtered mapstat.likelihood;obsfloattheta[0.25/3] Best core radius corresponding to the detectionarcminphys.angSize;srcfloatYSZ[4.1e-6/0.0005] Integrated Comptonization within a 0.75' aperturearcmin**2stat.fit.paramfloate_YSZ[3.4e-06/7.3e-05] Uncertainty in YSZarcmin**2stat.errorfloatz[0.05/1.7]? Redshiftsrc.redshiftfloatnullablee_z[0.015/0.2]? Uncertainty in zstat.error;src.redshiftfloatnullableM500[2.4/16]? Enclosed mass M500 without systematic errors (4)1e+14solMassphys.massfloatnullableE_M500[0.3/1.5]? Upper error in M5001e+14solMassstat.error;stat.maxfloatnullablee_M500[0.5/2]? Lower error in M5001e+14solMassstat.errorfloatnullableM200[4/24.7]? Enclosed mass M200 without systematic errors1e+14solMassphys.massfloatnullableE_M200[0.6/2.4]? Upper error in M2001e+14solMassstat.error;stat.maxfloatnullablee_M200[0.9/3]? Lower error in M2001e+14solMassstat.errorfloatnullableM500sys[2/15]? Enclosed mass M500 marginalized over systematic errors (5)1e+14solMassphys.massfloatnullableE_M500sys[0.4/2.3]? Upper error in M500sys1e+14solMassstat.error;stat.maxfloatnullablee_M500sys[0.6/3]? Lower error in M500sys1e+14solMassstat.errorfloatnullableM200sys[3.5/23.4]? Enclosed mass M200 marginalized over systematic errors1e+14solMassphys.massfloatnullableE_M200sys[0.6/3.6]? Upper error in M200sys1e+14solMassstat.error;stat.maxfloatnullablee_M200sys[1/4.8]? Lower error in M200sys1e+14solMassstat.errorfloatnullableSZCatDisplay data from Bayliss+ 2016, J/ApJS/227/3 and McDonald+, 2013, J/ApJ/774/23meta.ref.urlintnullableSimbadSimbad column added by the CDSmeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlchar