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相关论文: An X-ray Selected Galaxy Cluster at z=1.26

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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 discovery of a galaxy cluster at z=1.27. ClG J0848+4453 was found in a near-IR field survey as a high density region of objects with very red J-K colors. Optical spectroscopy of a limited number of 24 < R < 25 objects in the…

天体物理学 · 物理学 2009-10-30 S. A. Stanford , Richard Elston , Peter Eisenhardt , Hyron Spinrad , Daniel Stern , Arjun Dey

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 report the discovery of a massive, X-ray-luminous cluster of galaxies at z=1.393, the most distant X-ray-selected cluster found to date. XMMU J2235.3-2557 was serendipitously detected as an extended X-ray source in an archival XMM-Newton…

天体物理学 · 物理学 2011-09-30 C. R. Mullis , P. Rosati , G. Lamer , H. Boehringer , A. Schwope , P. Schuecker , R. Fassbender

We report on the discovery of a very distant galaxy cluster serendipitously detected in the archive of the XMM-Newton mission, within the scope of the XMM-Newton Distant Cluster Project (XDCP). XMMUJ0044.0-2033 was detected at a high…

We have obtained a new high-resolution K'-band image of the central region of the rich X-ray cluster RX J0848.9+4452 at z=1.26. We found that the brightest cluster galaxy (BCG) in the cluster is clearly separated into two distinct objects.…

天体物理学 · 物理学 2009-11-07 T. Yamada , Y. Koyama , F. Nakata , M. Kajisawa , I. Tanaka , T. Kodama , S. Okamura , R. De Propris

We report on the discovery of a galaxy cluster at z = 1.490 originally selected as an extended X-ray source in the XMM-Newton Distant Cluster Project. Further observations carried out with the VLT-FORS2 spectrograph allowed the…

We present a study of the galaxy population in the cluster RXJ0848+4453 at z=1.27, using deep HST NICMOS and WFPC2 images. We morphologically classify all galaxies to K_s=20.6 that are covered by the HST imaging, and determine photometric…

天体物理学 · 物理学 2009-11-06 P. G. van Dokkum , S. A. Stanford , B. P. Holden , P. R. Eisenhardt , M. Dickinson , R. Elston

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…

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

In the distant universe X-ray luminous clusters of galaxies are rare objects. Large area surveys are therefore needed to probe the high luminosity end of the cluster population at redshifts z >= 1. We correlated extended X-ray sources from…

天体物理学 · 物理学 2008-08-25 G. Lamer , M. Hoeft , J. Kohnert , A. Schwope , J. Storm

We present deep I, J_s, K_s imaging and optical spectroscopy of the newly discovered Red-Sequence Cluster Survey cluster RCS043938-2904.9. This cluster, drawn from an extensive preliminary list, was selected for detailed study on the basis…

An unusual double-lobed extended X-ray source (RX J105343+5735) is detected in the ROSAT ultra-deep HRI image of the Lockman Hole. The angular size of the source is 1.7 X 0.7 arcmin^2 and its X-ray flux is 2 X 10^-14 erg cm^-2 s^-1. R-band…

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

We present the largest sample of spectroscopically confirmed X-ray luminous high-redshift galaxy clusters to date comprising 22 systems in the range 0.9<z<\sim1.6 as part of the XMM-Newton Distant Cluster Project (XDCP). All systems were…

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 JKCS041, a massive near-infrared selected cluster of galaxies z=1.9. The cluster was originally discovered using a modified red-sequence method and was also detected in follow-up Chandra data as…

天体物理学 · 物理学 2015-05-13 S. Andreon , B. Maughan , G. Trinchieri , J. Kurk

We report the discovery of a galaxy cluster at z=1.62 located in the Spitzer Wide-Area Infrared Extragalactic survey XMM-LSS field. This structure was selected solely as an overdensity of galaxies with red Spitzer/IRAC colors, satisfying…

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…

宇宙学与河外天体物理 · 物理学 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

The Chandra X-ray Observatory was used to obtain a 190 ks image of three high redshift galaxy clusters in one observation. The results of our analysis of these data are reported for the two z > 1 clusters in this Lynx field, including the…

天体物理学 · 物理学 2016-08-30 S. A. Stanford , B. Holden , P. Rosati , P. Tozzi , S. Borgani , P. R. Eisenhardt , H. Spinrad

X-ray luminous clusters of galaxies at z~1 are emerging as major cosmological probes and are fundamental tools to study the cosmic large-scale structure and environmental effects of galaxy evolution at large look-back times. We present…

天体物理学 · 物理学 2009-11-13 R. Fassbender , H. Boehringer , G. Lamer , C. R. Mullis , P. Rosati , A. Schwope , J. Kohnert , J. S. Santos
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