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相关论文: A Lensed Arc in the Low Redshift Cluster Abell 212…

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We report on the serendipitous discovery in the Blanco Cosmology Survey (BCS) imaging data of a z = 0.9057 galaxy that is being strongly lensed by a massive galaxy cluster at a redshift of z=0.3838. The lens (BCS J2352-5452) was discovered…

We report on the detection of dark matter in the cluster Abell 2390 using the weak gravitational distortion of background galaxies. We find that the cluster light and total mass distributions are quite similar over an angular scale of…

天体物理学 · 物理学 2009-10-28 G. Squires , N. Kaiser , G. Fahlman , A. Babul , D. Woods

We discuss the statistical properties of faint background galaxies detected in a deep Hubble Space Telescope ultraviolet (F336W) Wide Field Planetary Camera 2 image of the lensing cluster Abell 370 (z=0.37). By combining modelled field…

天体物理学 · 物理学 2007-05-23 J. Bezecourt , G. Soucail , R. S. Ellis , J. -P. Kneib

We present a striking new Hubble Space Telescope (HST) observation of the rich cluster Abell 2218 taken with the Wide-Field and Planetary Camera (WFPC2). HST's restored image quality reveals a sizeable number of gravitationally-lensed…

天体物理学 · 物理学 2009-10-28 J. -P. Kneib , R. S. Ellis , I. Smail , W. J. Couch , R. M. Sharples

We present a weak lensing analysis of one of the most distant massive galaxy cluster known, RDCS 1252.9-2927 at z=1.24, using deep images from the Advanced Camera for Survey (ACS) on board the Hubble Space Telescope (HST). By taking…

A mass model of the rich cluster A2218 is presented based on optical and new near-infrared images of arc(let)s and the ROSAT/HRI X-ray map. A lensing model is proposed with two dark matter clumps, centered on the two bright galaxies around…

天体物理学 · 物理学 2008-02-03 J. -P. Kneib , Y. Mellier , R. Pello , J. Miralda-Escude , J. -F. Le Borgne , H. Bohringer , J. -P. Picat

Deep Hubble Space Telescope images of superlative resolution obtained for the distant rich cluster AC114 (z=0.31) reveal a variety of gravitational lensing phenomena for which ground-based spectroscopy is available. We present a luminous…

天体物理学 · 物理学 2009-10-22 Ian Smail , Warrick J. Couch , Richard S. Ellis , Ray M. Sharples

We present imaging and spectroscopic observations of the gravitationally lensed arcs in the field of RX J1347.5-1145, the most X-ray luminous galaxy cluster known. Based on the detection of the [OII] 3727 emission line, we confirm that the…

天体物理学 · 物理学 2009-11-07 Swara Ravindranath , Luis C. Ho

A unique reconstruction of the image of a high redshift source galaxy responsible for multiple long arcs in the z = 0.4 cluster 0024+1654 is obtained by inverse lensing. Deep B and I imaging with the Hubble Space Telescope (Based on…

天体物理学 · 物理学 2009-10-28 Wesley N. Colley , J. Anthony Tyson , Edwin L. Turner

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 report the discovery of an unusual emission line galaxy at redshift z=1.68 found from near-IR imaging and spectroscopic observations with ISAAC/VLT of a faint gravitationally lensed R-band drop-out behind the lensing cluster Abell 1835.…

天体物理学 · 物理学 2009-11-10 J. Richard , D. Schaerer , R. Pello , J. -F. Leborgne , J. -P. Kneib

We present a deep H-band image of the region in the vicinity of the cluster Abell 1942 containing the puzzling dark matter concentration detected in an optical weak lensing study by Erben et al. (2000). We demonstrate that our limiting…

天体物理学 · 物理学 2009-11-06 Meghan E. Gray , Richard S. Ellis , James R. Lewis , Richard G. McMahon , Andrew E. Firth

During our Herschel Lensing Survey (HLS) of massive galaxy clusters, we have discovered an exceptionally bright source behind the z=0.22 cluster Abell 773, which appears to be a strongly lensed submillimeter galaxy (SMG) at z=5.2429. This…

We present deep spectroscopic measurements of 18 distant field galaxies identified as gravitationally-lensed arcs in a Hubble Space Telescope image of the cluster Abell 2218. Redshifts of these objects were predicted by Kneib et al. (1996)…

We compare the statistical properties of giant gravitationally lensed arcs produced in matched simulated and observed cluster samples. The observed sample consists of 10 X-ray selected clusters at redshifts z ~ 0.2 imaged with HST by Smith…

天体物理学 · 物理学 2009-11-13 Assaf Horesh , Eran O. Ofek , Dan Maoz , Matthias Bartelmann , Massimo Meneghetti , Hans-Walter Rix

Abell 383 is a famous rich cluster (z = 0.1887) imaged extensively as a basis for intensive strong and weak lensing studies. Nonetheless there are few spectroscopic observations. We enable dynamical analyses by measuring 2360 new redshifts…

宇宙学与河外天体物理 · 物理学 2015-06-18 Margaret J. Geller , Ho Seong Hwang , Antonaldo Diaferio , Michael J. Kurtz , Dan Coe , Kenneth J. Rines

We report on the detection of dark matter in the cluster Abell 2218 using the weak gravitational distortion of background galaxies. We find a highly significant, coherent detection of the distortion in the images of the background galaxies.…

天体物理学 · 物理学 2009-10-28 G. Squires , N. Kaiser , A. Babul , G. Fahlman , D. Woods , D. M. Neumann , H. Böhringer

We identify a strong lensing galaxy in the cluster IRC 0218 (also known as XMM-LSS J02182$-$05102) that is spectroscopically confirmed to be at $z=1.62$, making it the highest-redshift strong lens galaxy known. The lens is one of the two…

We present the results of a dynamical analysis of the rich X-Ray luminous galaxy cluster Abell 521, and discuss the nature of the arc-like structure first noted by Maurogordato et al. (1996). Our study is based on radial velocities for 41…

天体物理学 · 物理学 2007-05-23 S. Maurogordato , D. Proust , T. C. Beers , M. Arnaud , R. Pello , A. Cappi , E. Slezak , J. Kriessler

We report on the discovery of three bright, strongly-lensed objects behind Abell 1703 and CL0024+16 from a dropout search over 25 square arcminutes of deep NICMOS data, with deep ACS optical coverage. They are undetected in the deep ACS…

宇宙学与河外天体物理 · 物理学 2010-01-15 W. Zheng , L. D. Bradley , R. J. Bouwens , H. C. Ford , G. D. Illingworth , N. Benitez , T. Broadhurst , B. Frye , L. Infante , M. J. Jee , V. Motta , X. W. Shu , A. Zitrin