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Related papers: The complex gravitational lens system B1933+503

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We model an apparent gravitational lens system HDFS 2232509-603243 in the Hubble Deep Field South. The system consists of a blue V=25 mag arc separated by 0.9 arcsec from a red V=22 mag elliptical galaxy. A mass distribution which follows…

Astrophysics · Physics 2009-10-31 Rennan Barkana , Roger Blandford , David Hogg

In the gravitational lens system B1600+434 the brighter image, A, is known to show rapid variability which is not detected in the weaker image, B (Koopmans & de Bruyn 2000). Since correlated variability is one of the fundamental properties…

Astrophysics · Physics 2009-11-06 Alok R. Patnaik , Athol J. Kemball

We report the discovery of a new gravitationally lensed quasar from the Sloan Digital Sky Survey, SDSS J090334.92+502819.2. This object was targeted for SDSS spectroscopy as a Luminous Red Galaxy (LRG), but manual examination of the…

We present near infrared observations of the red gravitational lens system MG0414+0534. Our images are of sufficient quality to allow photometry of all four QSO images and the lens galaxy. The observations show that the K-band brightnesses…

Astrophysics · Physics 2009-10-30 B. A. McLeod , G. M. Bernstein , M. J. Rieke , D. W. Weedman

We have produced deep radio maps of the double quasar 0957+561 from multiple-epoch VLA observations. To achieve high sensitivity to extended structure we have re-reduced the best available 1.6 GHz observations and have combined 5 GHz data…

Astrophysics · Physics 2009-10-30 I. M. Avruch , A. S. Cohen , J. Lehar , S. R. Conner , D. B. Haarsma , B. F. Burke

This is a short and biased review of gravitational lensing with emphasis on the radio and especially VLBI aspects. We briefly explain the basic idea and give a short sketch of the discovery of the first lens, before we more systematically…

Astrophysics · Physics 2007-10-11 Olaf Wucknitz

We present evidence that the optically unidentified radio source, FIRST J121839.7+295325, may be strongly lensing a background galaxy. We estimate the redshift of the assumed gravitational arc, discovered in parallel imaging with HST, from…

Astrophysics · Physics 2009-11-13 R. E. Ryan , S. H. Cohen , R. A. Windhorst , C. R. Keeton , T. J. Veach

The submillimeter galaxy (SMG) HERMES J105751.1+573027 (hereafter HLock01) at z = 2.9574 +/- 0.0001 is one of the brightest gravitationally lensed sources discovered in the Herschel Multi-tiered Extragalactic Survey. Apart from the high…

We have discovered strong gravitational lensing features in the core of the nearby cluster Abell 3827 by analyzing Gemini South GMOS images. The most prominent strong lensing feature is a highly-magnified, ring-shaped configuration of four…

Cosmology and Nongalactic Astrophysics · Physics 2010-05-17 E. R. Carrasco , P. L. Gomez , T. Verdugo , H. Lee , R. Diaz , M. Bergmann , J. E. H. Turner , B. W. Miller , M. J. West

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…

Strongly correlated non-intrinsic variability between 5 and 8.5 GHz has been observed in one of the lensed images of the gravitational lens B1600+434. These non-intrinsic (i.e. `external') variations are interpreted as `radio-microlensing'…

High angular resolution images of the complex gravitational lens system RXS J1131-1231 (a quadruply imaged AGN with a bright Einstein ring) obtained with the Advanced Camera for Surveys and NICMOS instruments onboard the Hubble Space…

Astrophysics · Physics 2009-11-11 J. -F. Claeskens , D. Sluse , P. Riaud , J. Surdej

The strange morphology of the six-component gravitational lens PMN J0134-0931 has resisted explanation. We present the first successful quantitative models for the system, based on the idea that there are two lens galaxies and two…

Astrophysics · Physics 2008-11-26 Charles R. Keeton , Joshua N. Winn

Galaxies located in the environment or on the line of sight towards gravitational lenses can significantly affect lensing observables, and can lead to systematic errors on the measurement of $H_0$ from the time-delay technique. We present…

While gravitationally lensed quasars are expected to display an odd number of images, invariably systems are observed with an even number of quasars. For this, lensing galaxies must have very small core radii; this provides strong…

We have found three gravitational lenses (two are new) by observing 34 likely FIRST radio lobes with APM galaxy counterparts. We expect to find $\sim30$ such lenses in over the next few years, which will significantly improve lensing…

Astrophysics · Physics 2007-05-23 J. Lehar , A. Buchalter , R. McMahon , C. Kochanek , D. Helfand , R. Becker , T. Muxlow

Discoveries of gamma-ray bursts (GRBs) have become commonplace in recent decades, totalling $\mathcal{O}(10^4)$ unique detections across various missions. However, there have been no confirmed discoveries of a gravitationally-lensed GRB,…

High Energy Astrophysical Phenomena · Physics 2026-04-09 Dan Ryczanowski , Benjamin P. Jones , Benjamin P. Gompertz , Graham P. Smith

We present a novel pilot search for gravitational lenses in the mJIVE-20 survey, which observed $24\,903$ radio sources selected from FIRST with the VLBA at an angular resolution of 5 mas. We have taken the visibility data for an initial…

Astrophysics of Galaxies · Physics 2018-12-19 C. Spingola , J. P. McKean , M. Lee , A. Deller , J. Moldon

We present Global VLBI and HSA images of the gravitational lens B2016+112 at 18, 6 and 3.6 cm. Previous VLBI observations showed that images A and B (which are clearly lensed images of a single background source) and the elongated region C…

Astrophysics · Physics 2007-05-23 A. More , R. W. Porcas

The gravitational lens configuration where a background galaxy is closely aligned with a foreground galaxy, can provide accurate measurement of the dark matter density profile in the foreground galaxy, free of dynamical assumptions.…

Astrophysics · Physics 2009-11-11 J. P. Willis , P. C. Hewett , S. J. Warren
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