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We present optical and near-infrared spectroscopic observations of the optical Einstein ring 0047-2808. We detect both [OIII] lines 4959, 5007 near 2.3 micron, confirming the redshift of the lensed source as z=3.595. The Ly-a line is…

天体物理学 · 物理学 2009-10-30 S. J. Warren , A. Iovino , P. C. Hewett , P. A. Shaver

In a previous paper, we outlined a new Bayesian method for inferring the properties of extended gravitational lenses, given data in the form of resolved images. This method holds the most promise for optimally extracting information from…

天体物理学 · 物理学 2008-11-26 Brendon J. Brewer , Geraint F. Lewis

MG 1131+0456 is a radio-selected gravitational lens, and is the first known Einstein ring. Discovered in 1988, the system consists of a bright radio source imaged into a ring and two compact, flat-spectrum components separated by 2.1…

星系天体物理 · 物理学 2020-12-21 Daniel Stern , Dominic Walton

We report the discovery of a partial Einstein ring of radius 1.48arcsec produced by a massive (and seemingly isolated) elliptical galaxy. The spectroscopic follow-up at the VLT reveals a 2L* galaxy at z=0.986, which is lensing a…

天体物理学 · 物理学 2007-05-23 R. A. Cabanac , D. Valls-Gabaud , A. O. Jaunsen , C. Lidman , H. Jerjen

We report an ultra-bright lensed submillimeter galaxy at $z_{spec}=1.4796$, identified as a result of a full-sky cross-correlation of the AllWISE and Planck compact source catalogs aimed to search for bright submillimeter galaxies at $z…

星系天体物理 · 物理学 2021-09-22 A. Díaz-Sánchez , H. Dannerbauer , N. Sulzenauer , S. Iglesias-Groth , R. Rebolo

(Abridged) We perform a detailed analysis of the optical gravitational lens ER 0047-2808 imaged with WFPC2 on the Hubble Space Telescope. Using software specifically designed for the analysis of resolved gravitational lens systems, we focus…

天体物理学 · 物理学 2008-11-26 Randall B. Wayth , Stephen J. Warren , Geraint F. Lewis , Paul C. Hewett

We report the discovery of an almost complete Einstein ring of diameter 10" in Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5). Spectroscopic data from the 6m telescope of the Special Astrophysical Observatory reveals that the…

We report the discovery of a new gravitational lens system from the CLASS survey, CLASS B0631+519. VLA, MERLIN and VLBA observations show a doubly-imaged radio core, a doubly-imaged lobe and a second lobe that is probably quadruply-imaged.…

We report on the discovery of a very bright z = 2.00 star-forming galaxy that is strongly lensed by a foreground z=0.422 luminous red galaxy (LRG). This system was found in a systematic search for bright arcs lensed by LRGs and brightest…

A deep spectrum taken with the Echelle Spectrograph and Imager (ESI) at the Keck II Telescope as part of the Lenses Structure and Dynamics (LSD) Survey reveals the redshifts of the extremely red source of the radio Einstein Ring in the…

天体物理学 · 物理学 2009-11-07 T. Treu , L. Koopmans

We present high resolution imaging of the low order (J=1 and 2) CO line emission from the z = 3.93 submillimeter galaxy (SMG) MM18423+5938 using the Expanded Very Large Array, and optical and near-IR imaging using the Canada-France-Hawaii…

星系天体物理 · 物理学 2015-05-28 J. -F. Lestrade , C. L. Carilli , Karun Thanjavur , J. -P. Kneib , D. A. Riechers , F. Bertoldi , F. Walter , A. Omont

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 a multi-wavelength study of the gravitational lens COSMOS J095930+023427 (z=0.89), together with the associated galaxy group located at $z\sim0.7$ along the line of sight and the lensed background galaxy. The source redshift is…

宇宙学与河外天体物理 · 物理学 2015-06-12 Shuo Cao , Giovanni Covone , Maurizio Paolillo , Zong-Hong Zhu

We have discovered strong gravitational lensing by the galaxy ESO325-G004, in images obtained with the Advanced Camera for Surveys on the Hubble Space Telescope. The lens galaxy is a boxy group-dominant elliptical at z=0.0345, making this…

天体物理学 · 物理学 2009-11-11 Russell J. Smith , John P. Blakeslee , John R. Lucey , John Tonry

We report the discovery of a very bright (r = 20.16), highly magnified, and yet intrinsically very luminous Ly{\alpha} emitter (LAE) at z = 2.82. This system comprises four images in the observer plane with a maximum separation of ~ 6" and…

The location of the images in a multiple-image gravitational lens system are strongly dependent on the orientation angle of the mass distribution. As such, we can use the location of the images and the photometric properties of the visible…

天体物理学 · 物理学 2007-05-23 Randall B. Wayth , Rachel L. Webster

(Abridged) We present our VLT/FORS1 deep spectroscopic observations of the gravitationally lensed quasar SDSS J0924+0219, as well as archival HST/NICMOS and ACS images of the same object. The two-epoch spectra, obtained in the Multi Object…

天体物理学 · 物理学 2009-11-11 A. Eigenbrod , F. Courbin , S. Dye , G. Meylan , D. Sluse , P. Saha , C. Vuissoz , P. Magain , .

We present new VLT observations of the closest-known strong-lensing galaxy, the sigma=330 km/s giant elliptical ESO325-G004. The low redshift of the lens (z_lens=0.035) results in arcs being formed at a small fraction of the effective…

宇宙学与河外天体物理 · 物理学 2015-06-16 Russell J. Smith , John R. Lucey

Using FORS2, mounted on Kueyen (UT2 of the VLT), we have obtained the redshift of the lensing galaxy in the gravitational lens system HE1104-1805. We measure z=0.729, in good agreement with previous estimates based on the time delay and the…

天体物理学 · 物理学 2007-05-23 C. Lidman , F. Courbin , J. -P. Kneib , G. Golse , F. Castander , G. Soucail
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