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We report 31 GHz CARMA observations of IDCS J1426.5+3508, an infrared-selected galaxy cluster at z = 1.75. A Sunyaev-Zel'dovich decrement is detected towards this cluster, indicating a total mass of M200 = (4.3 +/- 1.1) x 10^{14} Msun in…

We present a weak lensing study of the galaxy cluster IDCS J1426.5+3508 at $z=1.75$, which is the highest redshift strong lensing cluster known and the most distant cluster for which a weak lensing analysis has been undertaken. Using F160W,…

The galaxy cluster IDCS J1426.5+3508 at z = 1.75 is the most massive galaxy cluster yet discovered at z > 1.4 and the first cluster at this epoch for which the Sunyaev-Zel'Dovich effect has been observed. In this paper we report on the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Anthony H. Gonzalez , S. A. Stanford , Mark Brodwin , Cosimo Fedeli , Arjun Dey , Peter R. M. Eisenhardt , Conor Mancone , Daniel Stern , Greg Zeimann

We report the discovery of an IR-selected massive galaxy cluster in the IRAC Distant Cluster Survey (IDCS). We present new data from the Hubble Space Telescope and the W. M. Keck Observatory that spectroscopically confirm IDCS J1426+3508 at…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 S. A. Stanford , M. Brodwin , Anthony H. Gonzalez , Greg Zeimann , Daniel Stern , Arjun Dey , P. R. Eisenhardt , Gregory F. Snyder , C. Mancone

We report the discovery of XMMXCS J2215.9-1738, a massive galaxy cluster at z =1.45, which was found in the XMM Cluster Survey. The cluster candidate was initially identified as an extended X-ray source in archival XMM data. Optical…

(Abridged) We report the discovery of CXO J1415.2+3610, a distant (z~1.5) galaxy cluster serendipitously detected in a deep, high-resolution Chandra observation targeted to study the cluster WARP J1415.1+3612 at z=1.03. This is the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 P. Tozzi , J. S. Santos , M. Nonino , P. Rosati , S. Borgani , B. Sartoris , B. Altieri , M. Sanchez-Portal

We report the X-ray detection of two z>1.4 infrared-selected galaxy clusters from the IRAC Shallow Cluster Survey (ISCS). We present new data from the Hubble Space Telescope and the W. M. Keck Observatory that spectroscopically confirm…

We present an initial study of the mass and evolutionary state of a massive and distant cluster, RCS2 J232727.6-020437. This cluster, at z=0.6986, is the richest cluster discovered in the RCS2 project. The mass measurements presented in…

Galaxy clusters, being the largest gravitationally bound structures in the Universe, are a powerful tool to study mass assembly at different epochs. At z$>$2 they give an unique opportunity to put solid constraints not only on dark matter…

Galaxy clusters are the most massive gravitationally bound structures in the universe and serve as tracers of the assembly of large-scale structure. Studying their progenitors, proto-clusters, sheds light on the earliest stages of cluster…

Cosmology and Nongalactic Astrophysics · Physics 2026-01-29 Akos Bogdan , Gerrit Schellenberger , Qiong Li , Christopher J. Conselice

We report the discovery of a galaxy cluster at z = 1.41. ISCS J143809+341419 was found in the Spitzer/IRAC Shallow Survey of the Bootes field in the NOAO Deep Wide-Field Survey carried out by IRAC. The cluster candidate was initially…

Galaxy clusters trace the densest regions of the cosmic web and are crucial laboratories for studying the thermodynamic and chemical evolution of the intracluster medium (ICM). We present a Chandra study of the massive galaxy cluster SPT-CL…

Astrophysics of Galaxies · Physics 2026-01-14 Dan Hu , Shida Fan , Zhongsheng Yuan , Junjie Mao , Norbert Werner , Yuanyuan Su , François Mernier , Yuanyuan Zhao , Liyi Gu , Haiguang Xu

We present a weak-lensing analysis of the z=1.4 galaxy cluster XMMU J2235.3-2557, based on deep Advanced Camera for Surveys images. Despite the observational challenge set by the high redshift of the lens, we detect a substantial lensing…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 M. J. Jee , P. Rosati , H. C. Ford , K. S. Dawson , C. Lidman , S. Perlmutter , R. Demarco , V. Strazzullo , C. Mullis , H. Böhringer , R. Fassbender

We present a weak-lensing study of SPT-CLJ2040-4451 and IDCSJ1426+3508 at z=1.48 and 1.75, respectively. The two clusters were observed in our "See Change" program, a HST survey of 12 massive high-redshift clusters aimed at high-z supernova…

Cosmology and Nongalactic Astrophysics · Physics 2017-12-29 M. James Jee , Jongwan Ko , Saul Perlmutter , Anthony Gonzalez , Mark Brodwin , Eric Linder , Peter Eisenhardt

We present the results of a Chandra X-ray survey of the 8 most massive galaxy clusters at z>1.2 in the South Pole Telescope 2500 deg^2 survey. We combine this sample with previously-published Chandra observations of 49 massive…

We present resolved thermodynamic profiles out to 500 kpc, about $r_{500}$, of the $z=1.75$ galaxy cluster IDCS J1426.5+3508 with 40 kpc resolution. Thanks to the combination of Sunyaev-Zel'dovich and X-ray datasets, IDCS J1426.5+3508…

Cosmology and Nongalactic Astrophysics · Physics 2021-07-14 S. Andreon , C. Romero , F. Castagna , A. Ragagnin , M. Devlin , S. Dicker , B. Mason , T. Mroczkowski , C. Sarazin , J. Sievers , S. Stanchfield

We present a strong-lensing analysis of the galaxy cluster MS 1358.4+6245 ($z=0.33$), in deep 6-band ACS/HST imaging. In addition to the well-studied system at $z=4.92$, our modelling method uncovers 19 new multiply-lensed images so that a…

Cosmology and Nongalactic Astrophysics · Physics 2013-07-09 Adi Zitrin , Tom Broadhurst , Dan Coe , Jori Liesenborgs , Narciso Benitez , Yoel Rephaeli , Holland Ford , Keiichi Umetsu

We present details of the discovery of XLSSJ022303.0-043622, a z=1.2 cluster of galaxies. This cluster was identified from its X-ray properties and selected as a z>1 candidate from its optical/near-IR characteristics in the XMM Large-Scale…

We identify the largest known lensed images of a single spiral galaxy, lying close to the centre of the distant cluster MACS J1149.5+2223 ($z=0.544$). These images cover a total area of $\simeq 150 \Box\arcsec$ and are magnified $\simeq…

Cosmology and Nongalactic Astrophysics · Physics 2009-10-02 Adi Zitrin , Tom Broadhurst
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