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We present a 100 ks Chandra observation studying the extended X-ray emission around the powerful z=1.04 quasar PKS1229-021. The diffuse cluster X-ray emission can be traced out to ~15 arcsec (~120 kpc) radius and there is a drop in the…

宇宙学与河外天体物理 · 物理学 2015-06-03 H. R. Russell , A. C. Fabian , G. B. Taylor , J. S. Sanders , K. M. Blundell , C. S. Crawford , R. M. Johnstone , E. Belsole

We present a catalog of 200 clusters of galaxies serendipitously detected in 647 ROSAT PSPC pointings covering 158 square degrees. This is one of the largest X-ray selected cluster samples, comparable in size only to the ROSAT All-Sky…

天体物理学 · 物理学 2009-10-30 A. Vikhlinin. B. R. McNamara , W. Forman , C. Jones , H. Quintana , A. Hornstrup

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.…

宇宙学与河外天体物理 · 物理学 2025-09-03 Abigail Flowers , Jackson H. O'Donnell , Tesla E. Jeltema , Vernon Wetzell , M. Grant Roberts

A ROSAT HRI X-ray image was obtained of the open globular cluster NGC 288, which is located near the South Galactic Pole. This is the first deep X-ray image of this system. We detect a Low Luminosity Globular Cluster X-ray source (LLGCX)…

We report the detection of extended X-ray emission around several powerful 3CR quasars with redshifts out to 0.73. The ROSAT HRI images of the quasars have been corrected for spacecraft wobble and compared with an empirical point-spread…

天体物理学 · 物理学 2009-10-31 C. S. Crawford , I. Lehmann , A. C. Fabian , M. N. Bremer , G. Hasinger

Four compact ROSAT X-ray sources very close to the nearby ultraluminous infrared galaxy Arp 220 (IC 4553) have been identified as medium-redshift QSOs. The closest pair lying symmetrically across the galaxy have almost identical redshifts z…

天体物理学 · 物理学 2009-11-06 H. C. Arp , E. M. Burbidge , Y. Chu

We present photometric, spectroscopic and weak lensing analysis of the large-scale structure and dynamics of the most X-ray luminous galaxy cluster known, RX J1347-1145, at z=0.451. We spectroscopically confirmed 47 new members with LDSS3…

We have studied the spatial clustering of high redshift (z > 1) extremely red objects (EROs) as a function of photometric redshift in the GOODS Southern Field using public data. A remarkable overdensity of extremely red galaxies (I-Ks > 4)…

We present recent {\it Chandra} X-ray observations of the RXJ0821.0+0752 galaxy cluster in addition to ALMA observations of the CO(1-0) and CO(3-2) line emission tracing the molecular gas in its central galaxy. All of the CO line emission,…

Based on the ROSAT All-Sky Survey we have conducted a large redshift survey as an ESO key programme to identify and secure redshifts for the X-ray brightest clusters found in the southern hemisphere. We present first results for a highly…

Highly magnified lensed galaxies allow us to probe the morphological and spectroscopic properties of high-redshift stellar systems in great detail. However, such objects are rare, and there are only a handful of lensed galaxies which are…

天体物理学 · 物理学 2009-11-13 Eran O. Ofek , Stella Seitz , Felix Klein

We have observed the recently discovered rich star cluster GLIMPSE-C01 for 46 ks with the Chandra X-ray Observatory. Seventeen X-ray sources with luminosities greater than 0.6e31 ergs/s were discovered, one of which is likely a quiescent…

天体物理学 · 物理学 2007-08-27 D. Pooley , S. Rappaport , A. Levine , E. Pfahl , J. Schwab

We present radio through X-ray results of a bright (10^{40} erg/s in the 0.5 to 8.0 keV band) ultraluminous X-ray source (ULX), CXOU J153434.9+151149, in the starburst, interacting pair of galaxies NGC 5953/5954. Chandra image of this ULX…

天体物理学 · 物理学 2009-11-13 Margarita Rosado , Kajal K. Ghosh , Isaura Fuentes-Carrera

X-ray observations of clusters at different redshifts are presented and compared. For the nearest cluster -- the Virgo cluster -- we show a comparison of the galaxy distribution and the distribution of the intra-cluster gas. Although the…

天体物理学 · 物理学 2007-05-23 S. Schindler

We report evidence of a fully established galaxy cluster at z=2.07, consisting of a ~20sigma overdensity of red, compact spheroidal galaxies spatially coinciding with extended X-ray emission detected with XMM-Newton. We use VLT VIMOS and…

宇宙学与河外天体物理 · 物理学 2015-05-20 R. Gobat , E. Daddi , M. Onodera , A. Finoguenov , A. Renzini , N. Arimoto , R. Bouwens , M. Brusa , R. -R. Chary , A. Cimatti , M. Dickinson , X. Kong , M. Mignoli

Measurements of the velocities of galaxies thought to be associated with the giant radio galaxy NGC 6251 confirm the presence of a poor cluster with a systemic redshift of z= 0.0244 +/- 0.0004 and a line-of-sight velocity dispersion of…

天体物理学 · 物理学 2016-08-30 P. N. Werner , D. M. Worrall , M. Birkinshaw

Based on the ROSAT All-Sky Survey we are constructing a sample of the X-ray brightest galaxy clusters for cosmological studies. We have already completed the compilation of a sample of about 1000 clusters in the sky excluding a 40 degree…

天体物理学 · 物理学 2007-05-23 H. Boehringer , P. Schuecker , S. Komossa , J. Retzlaff , T. H. Reiprich , W. Voges

We present a catalog of spectroscopic redshifts for SPT-CLJ0615$-$5746, the most distant cluster in the Reionization Lensing Cluster Survey (RELICS). Using Nod & Shuffle multi-slit observations with LDSS-3 on Magellan, we identify…

星系天体物理 · 物理学 2019-06-19 Thomas Connor , Daniel D. Kelson , Guillermo A. Blanc , Konstantina Boutsia

We have analyzed the Chandra observation of the distant (z=0.164) galaxy cluster RXJ1720.1+2638 in which we find sharp features in the X-ray surface brightness on opposite sides of the X-ray peak: an edge at about 250 h_50^{-1} kpc to the…

天体物理学 · 物理学 2009-11-06 P. Mazzotta , M. Markevitch , A. Vikhlinin , W. R. Forman , L. P. David , L. VanSpeybroeck

We present the first detailed X-ray observations of optically-selected clusters at high redshift. Two clusters, Cl 1324+3011 at z = 0.76 and Cl 1604+4304 at z = 0.90, were observed with XMM-Newton. The optical center of each cluster is…

天体物理学 · 物理学 2009-11-10 Lori M. Lubin , John S. Mulchaey , Marc Postman