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We present a strong and weak lensing reconstruction of the massive cluster Abell 2744, the first cluster for which deep Hubble Frontier Field (HFF) images and spectroscopy from the Grism Lens-Amplified Survey from Space (GLASS) are…

We present a new high-precision, JWST-based, strong lensing model for the galaxy cluster Abell 2744 at $z=0.3072$. By combining the deep, high-resolution JWST imaging from the GLASS-JWST and UNCOVER programs and a Director's Discretionary…

We present a high-precision mass model of galaxy cluster Abell 2744, based on a strong-gravitational-lensing analysis of the \emph{Hubble Space Telescope Frontier Fields} (HFF) imaging data, which now include both \emph{Advanced Camera for…

We present the MUSE Hubble Ultra Deep Survey, a mosaic of nine MUSE fields covering 90\% of the entire HUDF region with a 10-hour deep exposure time, plus a deeper 31-hour exposure in a single 1.15 arcmin2 field. The improved observing…

The Hubble Frontier Fields (HFF) program combines the capabilities of the Hubble Space Telescope (HST) with the gravitational lensing of massive galaxy clusters to probe the distant Universe to an unprecedented depth. Here, we present the…

We conduct precise strong lensing mass modeling of four ${\it Hubble}$ Frontier Fields (HFF) clusters, Abell$~$2744, MACS$~$J0416.1$-$2403, MACS$~$J0717.5$+$3745, and MACS$~$J1149.6$+$2223, for which HFF imaging observations are completed.…

星系天体物理 · 物理学 2016-03-23 Ryota Kawamata , Masamune Oguri , Masafumi Ishigaki , Kazuhiro Shimasaku , Masami Ouchi

We present new observations of the lensing cluster SMACSJ2031.8-4036 obtained with the MUSE integral field spectrograph as part of its commissioning on the Very Large Telescope. By providing medium-resolution spectroscopy over the full…

宇宙学与河外天体物理 · 物理学 2015-06-22 J. Richard , V. Patricio , J. Martinez , R. Bacon , B. Clement , P. Weilbacher , K. Soto , L. Wisotzki , J. Vernet , R. Pello , J. Schaye , M. Turner , T. Martinsson

Parametric strong lensing studies of galaxy clusters often display "misleading features". This is the case in the galaxy cluster Abell 370. Using strong lensing techniques, it has been described parametrically by a four dark matter clumps…

Archival XMM and ROSAT X-ray data are used to investigate the structure of the Abell 548 - Abell 3367 region. Based on previous optical studies, this is a region likely to be rich in structure though studies are in disagreement regarding…

宇宙学与河外天体物理 · 物理学 2026-05-01 Mark J. Henriksen , Layla Ahmed

We present strong-lensing models, as well as mass and magnification maps, for the cores of the six HST Frontier Fields galaxy clusters. Our parametric lens models are constrained by the locations and redshifts of multiple image systems of…

宇宙学与河外天体物理 · 物理学 2015-06-19 Traci L. Johnson , Keren Sharon , Matthew B. Bayliss , Michael D. Gladders , Dan Coe , Harald Ebeling

We use a joint optical/X-ray analysis to constrain the geometry and history of the ongoing merging event in the massive galaxy cluster MACSJ0416.1-2403 (z=0.397). Our investigation of cluster substructure rests primarily on a combined…

Hubble Space Telescope imaging of the galaxy cluster Abell 1689 has revealed an exceptional number of strongly lensed multiply-imaged galaxies, including high-redshift candidates. Previous studies have used this data to obtain the most…

宇宙学与河外天体物理 · 物理学 2015-06-18 Jose M. Diego , T. Broadhurst , N. Benitez , K. Umetsu , D. Coe , I. Sendra , M. Sereno , L. Izzo , G. Covone

We present new VLT/MUSE observations of the Hubble Frontier Field (HFF) galaxy cluster MACS J1149.5+2223, lensing the well-known supernova "Refsdal" into multiple images, which enabled the first cosmological applications with a strongly…

宇宙学与河外天体物理 · 物理学 2024-09-05 S. Schuldt , C. Grillo , G. B. Caminha , A. Mercurio , P. Rosati , T. Morishita , M. Stiavelli , S. H. Suyu , P. Bergamini , M. Brescia , F. Calura , M. Meneghetti

We study the rotational motion of the galaxy cluster Abell 2107 at redshift z = 0.04 and its connection to nearby large-scale structures using a large amount of spectroscopic redshift data. By combining 978 new redshifts from the…

星系天体物理 · 物理学 2018-12-26 Hyunmi Song , Ho Seong Hwang , Changbom Park , Rory Smith , Maret Einasto

Strong gravitational lensing is a unique tool to model with great accuracy the inner mass distribution of massive galaxy clusters. In particular, clusters with large Einstein radii provide a wealth of multiply imaged systems in the cluster…

星系天体物理 · 物理学 2009-11-13 Johan Richard , Liuyi Pei , Marceau Limousin , Eric Jullo , Jean-Paul Kneib

We have conducted a two-layered spectroscopic survey (1'x1' ultra deep and 3'x3' deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUSE). The combination of a large field of view, high…

Magnetic fields in cluster outskirts and the intercluster medium are poorly constrained because diffuse synchrotron emission is hard to detect at low surface brightness. Faraday rotation measures (RMs) of polarized background sources can…

星系天体物理 · 物理学 2026-04-22 V. Gustafsson , M. Brüggen , C. Tasse , S. P. O'Sullivan

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

Extending over three Hubble Space Telescope (HST) cycles, the Hubble Frontier Fields (HFF) initiative constitutes the largest commitment ever of HST time to the exploration of the distant Universe via gravitational lensing by massive galaxy…

宇宙学与河外天体物理 · 物理学 2015-06-19 J. Richard , M. Jauzac , M. Limousin , E. Jullo , B. Clément , H. Ebeling , J. P. Kneib , H. Atek , P. Natarajan , E. Egami , R. Livermore , R. Bower

We present a gravitational lensing study of the massive galaxy cluster A2219 (redshift 0.22). This investigation is based on multicolour images from U through H, which allows photometric redshifts to be estimated for the background sources.…

天体物理学 · 物理学 2007-05-23 J. Bezecourt , H. Hoekstra , M. E. Gray , H. M. AbdelSalam , K. Kuijken , R. S. Ellis