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相关论文: A Spectroscopic Redshift for the Cl0024+16 Multipl…

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We present an optical analysis of a sample of 11 clusters built from the EXCPRES sample of X-ray selected clusters at intermediate redshift (z ~ 0.5). With a careful selection of the background galaxies we provide the mass maps…

宇宙学与河外天体物理 · 物理学 2015-09-02 Genevieve Soucail , Gael Foex , Etienne Pointecouteau , Monique Arnaud , Marceau Limousin

We investigate the possible existence of a high-redshift (z=1) cluster of galaxies associated with the QSO lens system MG2016+112. From an ultra-deep R- and less deep V- and I-band Keck images and a K-band mosaic from UKIRT, we detect ten…

天体物理学 · 物理学 2009-10-31 D. Clowe , N. Trentham , J. Tonry

Direct observations of the first generation of luminous objects will likely become feasible over the next decade. The advent of the Next Generation Space Telescope (NGST) will allow imaging of numerous galaxies and mini-quasars at redshifts…

天体物理学 · 物理学 2009-10-31 Rennan Barkana , Abraham Loeb

We present a strong and weak gravitational lens model of the galaxy cluster MACSJ0416.1-2403, constrained using spectroscopy from the Grism Lens-Amplified Survey from Space (GLASS) and Hubble Frontier Fields (HFF) imaging data. We search…

The knowledge of the redshift of multiple images in cluster-lenses allows to determine precisely the total projected mass within the Einstein radius. The observation of various multiple images in a same cluster is opening new possibilities…

天体物理学 · 物理学 2007-05-23 G. Golse , J. -P. Kneib , G. Soucail

We analyzed the spatial distribution of 28500 photometrically selected galaxies with AB magnitude 23.5<R<25.5 and redshift 1.4<z<3.5 in 21 fields with a total area of 0.81 square degrees. The galaxies were divided into three subsamples,…

天体物理学 · 物理学 2009-11-10 K. L. Adelberger , C. C. Steidel , M. Pettini , A. E. Shapley , N. A. Reddy , D. K. Erb

In this Letter we present a detailed study of the lensing configuration in the cluster Abell 2218. Four multiple-images systems with measured spectroscopic redshifts have been identified in this cluster. These multiple images are very…

天体物理学 · 物理学 2009-11-10 G. Soucail , J. P. Kneib , G. Golse

We present a weak lensing analysis of the X-ray luminous cluster CL 0152-1357 at z~0.84 using HST/ACS observations. The unparalleled resolution and sensitivity of ACS enable us to measure weakly distorted, faint background galaxies to the…

天体物理学 · 物理学 2014-10-13 M. J. Jee , R. L. White , N. Benitez , H. C. Ford , J. P. Blakeslee , P. Rosati , R. Demarco , G. D. Illingworth

We present a new high-precision strong lensing model of PLCK G287.0$+$32.9, a massive lens galaxy cluster at $z=0.383$, with the aim to get an accurate estimation of its effective Einstein radius and total mass distribution. We also present…

Gravitational lensing is an important tool for probing the mass distribution of galaxies. In this letter we report the discovery of a new quadruple lens HST 1411+5211 found in archived WFPC2 images of the galaxy cluster CL140933+5226. If…

天体物理学 · 物理学 2009-10-30 Philippe Fischer , David Schade , Felipe Barientos

We present joint X-ray and optical observations of the high redshift (z~0.83) lensing cluster CLJ0152.7-1357 made with the Chandra X-ray Observatory and the Keck telescope. We confirm the existence of significant substructure at both X-ray…

天体物理学 · 物理学 2015-06-24 Zhi-Ying Huo , Sui-Jian Xue , Haiguang Xu , Gordon Squires , Piero Rosati

We present an image of the redshift 2.3 IRAS source FSC10214+4724 at 0.8 microns obtained with the HST WFPC2 Planetary Camera. The source appears as an unresolved (< 0.06") arc 0.7" long, with significant substructure along its length. The…

天体物理学 · 物理学 2009-10-28 Peter R. Eisenhardt , Lee Armus , David W. Hogg , B. T. Soifer , G. Neugebauer , Michael W. Werner

We present new spectroscopic observations of the gravitational arcs and the brightest cluster galaxy (BCG) in the cluster MS2137-23 (z=0.313) obtained with the Echelle Spectrograph and Imager on the Keck II telescope. We find that the…

天体物理学 · 物理学 2009-11-07 David J. Sand , Tommaso Treu , Richard S. Ellis

Low-resolution spectrographs used to have difficulties to determine redshifts of galaxies at $z\approx1$ and $z\approx3$. Spectral emission and absorption lines of magnesium and iron redshifted to $z\approx1$ fall close to hydrogen,…

星系天体物理 · 物理学 2026-04-23 Jenny Wagner , Richard E. Griffiths , Emilio E. Falco

We outline a simple procedure designed for \emph{automatically} finding sets of multiple images in strong lensing (SL) clusters. We show that by combining (a) an arc-finding (or source extracting) program, (b) photometric redshift…

宇宙学与河外天体物理 · 物理学 2020-01-08 Mauricio Carrasco , Adi Zitrin , Gregor Seidel

We present a detailed velocity histogram from a wide-field spectroscopic survey in the field of the cluster lens Cl0024 showing an unrelaxed foreground structure in addition to the relaxed main cluster. This finding reduces the velocity…

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

This paper presents 52 X-ray bright galaxy clusters selected within the 11 deg$^2$ XMM-LSS survey. 51 of them have spectroscopic redshifts ($0.05<z<1.06$), one is identified at $z_{\rm phot}=1.9$, and all together make the high-purity…

宇宙学与河外天体物理 · 物理学 2015-06-22 N. Clerc , C. Adami , M. Lieu , B. Maughan , F. Pacaud , M. Pierre , T. Sadibekova , G. P. Smith , P. Valageas , B. Altieri , C. Benoist , S. Maurogordato , J. P. Willis

We present an HST/ACS weak gravitational lensing analysis of 13 massive high-redshift (z_median=0.88) galaxy clusters discovered in the South Pole Telescope (SPT) Sunyaev-Zel'dovich Survey. This study is part of a larger campaign that aims…

The gravitational potential responsible for the lensing effect in SBS 1520+530 is studied over length scales from a few arc-seconds to a few arc-minutes. For this purpose, we use sharply deconvolved Hubble Space Telescope images in the…

天体物理学 · 物理学 2009-11-07 C. Faure , F. Courbin , J. P. Kneib , D. Alloin , M. Bolzonella , I. Burud