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In this paper, we present new determinations of redshifts on a sample of gravitational arclets identified in the cluster of galaxies Abell 2390. The arclets candidates were selected from their elongated morphology as seen in recent deep HST…

天体物理学 · 物理学 2007-05-23 J. Bezecourt , G. Soucail

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

We report the discovery of an arc-like object 27" from the center of the cD galaxy in the redshift $z=0.066$ cluster A2124. Observations with the Keck II telescope reveal that the object is a background galaxy at $z=0.573$, apparently…

天体物理学 · 物理学 2009-10-30 John P. Blakeslee , Mark R. Metzger

Strong lensing by massive galaxy clusters can provide magnification of the flux and even multiple images of the galaxies that lie behind them. This phenomenon facilitates observations of high-redshift supernovae (SNe), that would otherwise…

星系天体物理 · 物理学 2018-07-04 T. Petrushevska , A. Goobar , D. J. Lagattuta , R. Amanullah , L. Hangard , S. Fabbro , C. Lidman , K. Paech , J. Richard , J. P. Kneib

We report the discovery of a unique $z=6.027$ galaxy, multiply imaged by the cluster Abell 383 and detected in new Hubble Space Telescope ACS and WFC3 imaging, as well as in Warm Spitzer observations. This galaxy was selected as a pair of…

宇宙学与河外天体物理 · 物理学 2015-05-27 Johan Richard , Jean-Paul Kneib , Harald Ebeling , Dan Stark , Eiichi Egami , Andrew K. Fiedler

We explore for the first time the possibility of detecting lensed star transients in galaxy-galaxy strong lensing systems upon repeated, deep imaging using the {\it James-Webb Space Telescope} ({\it JWST}). Our calculation predicts that the…

We discuss the optical spectrum of a multiply-imaged arc resolved by HST in the $z$=0.175 cluster A2218. The spectrum, obtained with LDSS-2 on the 4.2m William Herschel telescope, reveals the source to be a galaxy at a redshift $z$=2.515 in…

天体物理学 · 物理学 2016-06-08 T. M. D. Ebbels , J. -F. Le Borgne , R. Pelló , R. S. Ellis , J. -P. Kneib , I. Smail , B. Sanahuja

We report the discovery of four extremely faint ($m_{\mathrm{F444W}}\gtrsim29$) red point sources in recent ultra-deep JWST/NIRCam images of the strong lensing galaxy cluster Abell S1063. All four sources sit in lensed arcs, on the symmetry…

We discuss the physical nature of a remarkably faint pair of Lyman alpha-emitting images discovered close to the giant cD galaxy in the lensing cluster Abell 2218 (z=0.18) during a systematic survey for highly-magnified star-forming…

天体物理学 · 物理学 2009-11-07 Richard Ellis , Mike Santos , Jean-Paul Kneib , Konrad Kuijken

We present redshift measurements of four faint galaxies around the archetypal ultraluminous infrared galaxy Arp 220. These galaxies have significantly higher redshifts ($z \sim$ 0.036 -- 0.091) than that of Arp 220 ($z \simeq 0.018$).…

天体物理学 · 物理学 2009-10-31 Youichi Ohyama , Yoshiaki Taniguchi , J. E. Hibbard , William D. Vacca

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

In a recent paper Pello et al. reported observations of a faint galaxy, gravitationally lensed by the galaxy cluster Abell 1835. Deep J-band spectroscopy revealed a weak emission line near 1.34 microns, detected in two spectra with…

天体物理学 · 物理学 2014-10-13 S. J. Weatherley , S. J. Warren , T. S. R. Babbedge

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…

A massive galaxy cluster can serve as a magnifying glass for distant stellar populations, with strong gravitational lensing exposing details in the lensed background galaxies that would otherwise be undetectable. The MACS J0416.1-2403…

We examine a caustic-straddling arc at $z=0.9397$ in the field of the galaxy cluster MACS J0416.1-2403 ($z=0.397$) using archival multiband HST images and show that its surface brightness exhibits anomalies that can be explained by a single…

星系天体物理 · 物理学 2019-07-31 Alexander A. Kaurov , Liang Dai , Tejaswi Venumadhav , Jordi Miralda-Escudé , Brenda Frye

We report the first likely spectroscopic confirmation of a z 10.0 galaxy from our ongoing search for distant galaxies with ISAAC/VLT. Galaxy candidates at z >~ 7 are selected from ultra-deep JHKs images in the core of gravitational lensing…

天体物理学 · 物理学 2014-10-13 R. Pello , D. Schaerer , J. Richard , J. -F. Le Borgne , J. -P. Kneib

We report on Spitzer IRAC observations of the spectroscopically confirmed z=6.56 lensed Ly-alpha emitting source HCM 6A which was found behind the cluster Abell 370. Detection of the source at 3.6 and 4.5 microns, corresponding to…

天体物理学 · 物理学 2009-11-13 Ranga-Ram Chary , Daniel Stern , Peter Eisenhardt

We analyze the seldomly discussed lensing effects expected in low-z clusters (z = 0.05-0.15), using as an example the bright arc (z=0.073) discovered by Campusano and Hardy(1996) near the dominant cD galaxy of the cluster Abell 3408…

天体物理学 · 物理学 2009-10-30 Luis E. Campusano , Jean-Paul Kneib , Eduardo Hardy

The Reionization Cluster Survey (RELICS) imaged 41 galaxy clusters with the Hubble Space Telescope (HST), in order to detect lensed and high-redshift galaxies. Each cluster was imaged to about 26.5 AB mag in three optical and four…

Once only accessible in nearby galaxies, we can now study individual stars across much of the observable universe aided by galaxy-cluster gravitational lenses. When a star, compact object, or multiple such objects in the foreground…