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We present a multi-wavelength study of RX J0848+4456, a cluster of galaxies discovered through X-ray emission in the ROSAT Deep Cluster Survey. Our observations consist of WFPC2 imaging, optical spectra, and X-ray data collected with the…

We present a sample of 47 spectroscopically confirmed members of RX J1347-1145, the most luminous X-ray cluster of galaxies discovered to date. With two exceptions, all the galaxies in this sample have red B-R colors and red spectral…

天体物理学 · 物理学 2009-11-07 Judith G. Cohen , Jean-Paul Kneib

Clusters of galaxies at redshifts nearing one are of special importance since they may be caught at the epoch of formation. At these high redshifts there are very few known clusters. We present follow-up ASCA, ROSAT HRI and Keck LRIS…

天体物理学 · 物理学 2009-10-31 I. M. Gioia , J. P. Henry , C. R. Mullis , H. Ebeling , A. Wolter

An analysis of a ROSAT/HRI observation of the optically rich, gravitationally lensing galaxy cluster CL0500-24 (or Abell S0506) is presented. We show that the X-ray luminosity of this supposedly rich cluster is relatively low at…

天体物理学 · 物理学 2007-05-23 Sabine Schindler , Joachim Wambsganss

Galaxy cluster mass distribution are potentially useful probes of $\Omega_0$ and the nature of the dark matter. Large clusters will distort the observed shapes of background galaxies through gravitational lensing allowing the measurement of…

天体物理学 · 物理学 2016-08-30 Philippe Fischer , J. Anthony Tyson

We report on the discovery of the z=1.016 cluster RzCS 052 using a modified red sequence method, followup spectroscopy and X-ray imaging. This cluster has a velocity dispersion of 710+-150 km/s, a virial mass of 4.0e14 Msol (based on 21…

天体物理学 · 物理学 2009-11-13 S. Andreon , R. De Propris , E. Puddu , L. Giordano , H. Quintana

We present the results of a search for X--ray luminous distant clusters of galaxies. We found extended X--ray emission characteristic of a cluster towards two of our candidate clusters of galaxies. They both have a luminosity in the ROSAT…

天体物理学 · 物理学 2009-10-22 R. C. Nichol , M. P. Ulmer , R. G. Kron , G. D. Wirth , D. C. Koo

Using deep Chandra and optical spectroscopic observations, we investigate an intriguing, young massive group, RXJ1648.7+6109, at z=0.376, and we combine these observations with previous measurements to fit the scaling relations of…

天体物理学 · 物理学 2010-11-11 T. E. Jeltema , J. S. Mulchaey , L. M. Lubin

Large-scale fluctuations of the X-ray background are investigated using the ROSAT All-Sky Survey. The autocorrelation function of the extragalactic background at 1 keV is determined at separations 0.1 - 40 deg. We detect a significant…

天体物理学 · 物理学 2007-05-23 Andrzej M. Soltan , Guenther Hasinger , Roland Egger , Steve Snowden , Joachim Truemper

We present an analysis of the X-ray emission for a complete sample of 288 Abell clusters spanning the redshift range 0.016<= z <= 0.09 from the ROSAT All-Sky Survey. This sample is based on our 20cm VLA survey of nearby Abell clusters. We…

天体物理学 · 物理学 2009-11-10 Michael J. Ledlow , Wolfgang Voges , Frazer N. Owen , Jack O. Burns

We present spectroscopic confirmation of nine moderate redshift galaxy groups and poor clusters selected from the ROSAT Deep Cluster Survey. The groups span the redshift range z=0.23-0.59 and have between 4 and 20 confirmed members. The…

天体物理学 · 物理学 2009-11-11 John S. Mulchaey , Lori M. Lubin , Chris Fassnacht , Piero Rosati , Tesla E. Jeltema

We study the properties of the fossil cluster RX J1416.4+2315 through g' and i'-band imaging and spectroscopy of 25 member galaxies. The system is at a mean redshift of 0.137 and has a velocity dispersion of 584 km s^-1. Superimposed onto…

天体物理学 · 物理学 2008-11-26 Eduardo S. Cypriano , Claudia L. Mendes de Oliveira , Laerte Sodré

We report the detection of a massive high-redshift cluster of galaxies near the quadruple quasar RX J0911+05, using the LRIS instrument on the Keck-II telescope. The cluster is found to have a mean redshift of <z>=0.7689+/-0.002 and a…

天体物理学 · 物理学 2007-05-23 Jean-Paul Kneib , Judith G. Cohen , Jens Hjorth

We present X-ray observations of the narrow line radio galaxy 1138-262 at z = 2.156 with the High Resolution Imager (HRI) on ROSAT. Observations at other wave-bands, and in particular extremely high values of Faraday rotation of the…

天体物理学 · 物理学 2015-06-24 C. L. Carilli , D. E. Harris , L. Pentericci , H. J. A. Rottgering , G. K. Miley , M. N. Bremer

We have measured the surface density of galaxies toward 14 X-ray-selected cluster candidates at redshifts greater than z=0.46, and we show that they are associated with rich galaxy concentrations. We find that the clusters range between…

天体物理学 · 物理学 2009-11-06 B. R. McNamara , A. Vikhlinin , A. Hornstrup , H. Quintana , K. Whitman , W. Forman , C. Jones

We present the revised catalog of galaxy clusters detected as extended X-ray sources in the 160 Square Degree ROSAT Survey, including spectroscopic redshifts and X-ray luminosities for 200 of the 201 members. The median redshift is z~0.25…

We report the discovery of an X-ray luminous galaxy cluster at z =1.11. RDCS J0910+5422 was selected as an X-ray cluster candidate in the ROSAT Deep Cluster Survey on the basis of its spatial extent in a Rosat PSPC image. Deep optical and…

天体物理学 · 物理学 2009-11-07 S. A. Stanford , B. P. Holden , P. Rosati , P. R. Eisenhardt , D. Stern , G. Squires , H. Spinrad

We report the detection of weak gravitational lensing of distant background galaxies by two rich, X-ray luminous clusters of galaxies, MS 1137+66 at z=0.783 and RXJ 1716+67 at z=0.813. We detect a shear signal in each cluster over the…

天体物理学 · 物理学 2009-09-25 D. Clowe , N. Kaiser , G. Luppino , J. P. Henry , I. M. Gioia

We report the discovery of an X-ray luminous galaxy cluster at z=1.26. RXJ0848.9+4452 was selected as an X-ray cluster candidate in the ROSAT Deep Cluster Survey, on the basis of its spatial extent. Deep optical and near-IR imaging have…

We present the results of an extensive spectroscopic survey of RX J0152.7-1357, one of the most massive distant clusters of galaxies known. Multi-object spectroscopy, carried out with FORS1 and FORS2 on the ESO Very Large Telescope (VLT),…

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