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We present a sample of over 100 highly X-ray luminous galaxy clusters at $z\sim$ 0.5-0.9, discovered by the extended Massive Cluster Survey (eMACS) in ROSAT All-Sky Survey (RASS) data. Follow-up observations of a subset at higher resolution…

Cosmology and Nongalactic Astrophysics · Physics 2024-04-19 H. Ebeling , J. Richard , B. Beauchesne , Q. Basto , A. C. Edge , I. Smail

We present results of a combined X-ray/optical analysis of the dynamics of the massive cluster MACS J0358.8-2955 (z=0.428) based on observations with the Chandra X-ray Observatory, the Hubble Space Telescope, and the Keck-I telescope on…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Li-Yen Hsu , Harald Ebeling , Johan Richard

The WARPS team reviews the properties and history of discovery of ClJ0152.7-1357, an X-ray luminous, rich cluster of galaxies at z=0.833. At L_X = 8 x 10^44 h^(-2) erg/s (0.5-2.0 keV) ClJ0152.7-1357 is the most X-ray luminous cluster known…

Astrophysics · Physics 2009-10-31 H. Ebeling , L. R. Jones , E. Perlman , C. Scharf , D. Horner , G. Wegner , M. Malkan , B. Fairley , C. R. Mullis

We model the total mass and galactic substructure in the strong lensing galaxy cluster MACS J0138.0-2155 using a combination of Chandra X-ray data, Multi-Unit Spectroscopic Explorer (MUSE) spectroscopy, and Hubble Space Telescope imaging.…

Cosmology and Nongalactic Astrophysics · Physics 2025-09-03 Abigail Flowers , Jackson H. O'Donnell , Tesla E. Jeltema , Vernon Wetzell , M. Grant Roberts

We present results of a strong-lensing analysis of MACS J0717.5+3745 (hereafter MACS J0717), an extremely X-ray luminous galaxy cluster at z=0.55. Observations at different wavelengths reveal a complex and dynamically very active cluster,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 M. Limousin , H. Ebeling , J. Richard , A. M. Swinbank , G. P. Smith , M. Jauzac , S. Rodionov , C. -J. Ma , I. Smail , A. C. Edge , E. Jullo , J. P. Kneib

By constructing scaling relations for galaxies in the massive cluster MACSJ0717.5 at $z=0.545$ and comparing with those of Coma, we model the luminosity evolution of the stellar populations and the structural evolution of the galaxies. We…

Astrophysics of Galaxies · Physics 2016-12-21 L. J. Oldham , R. C. W. Houghton , Roger L. Davies

We report the discovery of a very bright (m_R = 22.2) Lyman break galaxy at z = 3.03 that appears to be a massive system in a late stage of merging. Deep imaging reveals multiple peaks in the brightness profile with angular separations of…

We investigate the physical properties, geometry and dynamics of the massive cluster merger MACS J0140.0-0555 (z=0.451) using X-ray and optical diagnostics. Featuring two galaxy overdensities separated by about 250 kpc in projection on the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 I-Ting Ho , Harald Ebeling , Johan Richard

We present the statistically complete and cosmologically most relevant subset of the twelve most distant galaxy clusters detected at z>0.5 by the MAssive Cluster Survey (MACS). Ten of these systems are new discoveries; only two…

Astrophysics · Physics 2009-11-13 H. Ebeling , E. Barrett , D. Donovan , C. -J. Ma , A. C. Edge , L. van Speybroeck

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…

We present JWST observations of the environments surrounding two high-redshift quasars, J0252$-$0503 at $z = 7.0$ and J1007$+$2115 at $z = 7.5$, which enable the first constraints on quasar-galaxy clustering at $z \sim 7.3$. Galaxies in the…

We present the results of a multiwavelength investigation of the very X-ray luminous galaxy cluster MACSJ0553.4-3342 ($z = 0.4270$; hereafter MACSJ0553). Combining high-resolution data obtained with the Hubble Space Telescope and the…

Cosmology and Nongalactic Astrophysics · Physics 2017-10-23 Harald Ebeling , Jia Qi , Johan Richard

We present results from a dynamical study of the high redshift, massive, X-ray luminous galaxy cluster MS1054--03. We significantly increase the number of confirmed cluster members by adding 20 to an existing set of twelve; using the…

We present Advanced Camera for Surveys observations of MACSJ1149.5+2223, an X-ray luminous galaxy cluster at z=0.544 discovered by the Massive Cluster Survey. The data reveal at least seven multiply-imaged galaxies, three of which we have…

We analyze a rich dataset including Subaru/SuprimeCam, HST/ACS and WFC3, Keck/DEIMOS, Chandra/ACIS-I, and JVLA/C and D array for the merging galaxy cluster ZwCl 0008.8+5215. With a joint Subaru/HST weak gravitational lensing analysis, we…

Astrophysics of Galaxies · Physics 2017-04-05 Nathan Golovich , Reinout J. van Weeren , William A. Dawson , M. James Jee , David Wittman

We discuss the X-ray and optical properties of the massive galaxy cluster MACSJ1206.2-0847 (z=0.4385), discovered in the Massive Cluster Survey (MACS). Our Chandra observation of the system yields a total X-ray luminosity of 2.4 x 10^45…

High Energy Astrophysical Phenomena · Physics 2009-11-13 H. Ebeling , C. J. Ma , J. -P. Kneib , E. Jullo , N. J. D. Courtney , E. Barrett , A. C. Edge , J. -F. Le Borgne

MACS J0600.1-2008 (MACS0600) is an X-ray luminous, massive galaxy cluster at $z_{\mathrm{d}}=0.43$, studied previously by the REionization LensIng Cluster Survey (RELICS) and ALMA Lensing Cluster Survey (ALCS) projects which revealed a…

We present a detailed kinematical and dynamical study of the galaxy cluster RXCJ1111.6+4050 (RXCJ1111), at z = 0.0756 using 104 new spectroscopic redshifts of galaxies observed at the TNG 3.5m telescope and SDSS DR16 public archive. Our…

Cosmology and Nongalactic Astrophysics · Physics 2023-11-29 R. Barrena , G. Chon , H. Böhringer , J. Méndez-Abreu , A. Ferragamo

We present the strong lensing analysis of two galaxy clusters: MACS J0242.5-2132 (MACS J0242, $z=0.313$) and MACS J0949.8+1708 (MACS J0949, $z=0.383$). Their total matter distributions are constrained thanks to the powerful combination of…

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