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The quasar SDSS J133401.39+331534.3 at z = 2.426 is found to be a two-image gravitationally lensed quasar with the image separation of 0.833. The object is first identified as a lensed quasar candidate in the Sloan Digital Sky Survey Quasar…

We report the results of an optical spectroscopic follow-up of four double quasar candidates in the Sloan Digital Sky Survey (SDSS) database. SDSS J1617+3827 is most likely a lensed quasar at z = 2.079, consisting of two images with r ~…

Astrophysics of Galaxies · Physics 2018-08-08 V. N. Shalyapin , A. V. Sergeyev , L. J. Goicoechea , A. P. Zheleznyak

We report the discovery of a new double image gravitational lens system B1030+074 which was found during the Jodrell Bank - VLA Astrometric Survey (JVAS). We have collected extensive radio data on the system using the VLA, MERLIN, the EVN…

The discovery of a gravitational lens candidate is reported. The quasars SDSS J111611.73+411821.5 and SDSS J111610.68+411814.4 are recognized as two images of the same object, being strongly lensed by the closer galaxy SDSS…

Astrophysics · Physics 2007-05-23 E. Sanchez Alvaro , F. J. Rodriguez Calonge

We construct a high resolution mass map of the z=0.39 cluster 0024+1654, based on parametric inversion of the associated gravitational lens. The lens creates eight well-resolved sub-images of a background galaxy, seen in deep imaging with…

Astrophysics · Physics 2009-10-30 J. Anthony Tyson , Greg P. Kochanski , Ian P. Dell'Antonio

We present our lens mass model of SMACS J0723, the first strong gravitational lens observed by the James Webb Space Telescope (JWST). We use data from the Hubble Space Telescope and Multi Unit Spectroscopic Explorer (MUSE) to build our…

Astrophysics of Galaxies · Physics 2022-10-14 G. B. Caminha , S. H. Suyu , A. Mercurio , G. Brammer , P. Bergamini , E. Vanzella , A. Acebron

We report the discovery of a pair of quasars at $z=1.487$, with a separation of $8\farcs585\pm0\farcs002$. Subaru Telescope infrared imaging reveals the presence of an elliptical and a disk-like galaxy located almost symmetrically between…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Cristian E. Rusu , Masamune Oguri , Masanori Iye , Naohisa Inada , Issha Kayo , Min-Su Shin , Dominique Sluse , Michael A. Strauss

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…

We report the results from a study of two massive ($M_{500c} > 6.0 \times 10^{14} M_{\odot}$) strong lensing clusters selected from the South Pole Telescope cluster survey for their high Einstein radius ($R_E > 40''$), SPT-CLJ2325$-$4111…

We compute the expected number of quasars multiply imaged by cluster size dark halos for current wide field quasar surveys by carrying out a large ensemble of ray tracing simulations through clusters from a cosmological N-body simulation of…

Astrophysics · Physics 2008-11-26 Joseph F. Hennawi , Neal Dalal , Paul Bode

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

We present a striking new Hubble Space Telescope (HST) observation of the rich cluster Abell 2218 taken with the Wide-Field and Planetary Camera (WFPC2). HST's restored image quality reveals a sizeable number of gravitationally-lensed…

Astrophysics · Physics 2009-10-28 J. -P. Kneib , R. S. Ellis , I. Smail , W. J. Couch , R. M. Sharples

HST V and I-band observations show that the gravitational lens B1359+154 consists of six images of a single z_s=3.235 radio source and its star-forming host galaxy, produced by a compact group of galaxies at z_l = 1. VLBA observations at…

We report the detection of a massive high-redshift cluster of galaxies near the quadruple quasar RX J0911+05, using the LRIS instrument on the Keck-II telescope. The cluster is found to have a mean redshift of <z>=0.7689+/-0.002 and a…

Astrophysics · Physics 2007-05-23 Jean-Paul Kneib , Judith G. Cohen , Jens Hjorth

We present a weak-lensing analysis of the z=1.4 galaxy cluster XMMU J2235.3-2557, based on deep Advanced Camera for Surveys images. Despite the observational challenge set by the high redshift of the lens, we detect a substantial lensing…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 M. J. Jee , P. Rosati , H. C. Ford , K. S. Dawson , C. Lidman , S. Perlmutter , R. Demarco , V. Strazzullo , C. Mullis , H. Böhringer , R. Fassbender

We present the first result of a survey for strong galaxy-galaxy lenses in Sloan Digital Sky Survey (SDSS) images. SDSS J082728.70+223256.4 was selected as a lensing candidate using selection criteria based on the color and positions of…

We present a combined strong and weak lensing analysis of the J085007.6+360428 (J0850) field, which was selected by its high projected concentration of luminous red galaxies and contains the massive cluster Zwicky 1953. Using…

We present a new strong lensing (SL) model of the Hubble Frontier Fields galaxy cluster Abell 2744, at z=0.3072, by exploiting archival Hubble Space Telescope (HST) multi-band imaging and Multi Unit Spectroscopic Explorer (MUSE) follow-up…

Cosmology and Nongalactic Astrophysics · Physics 2023-02-08 P. Bergamini , A. Acebron , C. Grillo , P. Rosati , G. B. Caminha , A. Mercurio , E. Vanzella , G. Angora , G. Brammer , M. Meneghetti , M. Nonino

An observation of the gravitationally lensed system 2016+112 with the Chandra X-ray Observatory has resolved a mystery regarding the proposed presence of a dark matter object in the lens plane of this system. The Chandra ACIS observation…

Astrophysics · Physics 2009-11-06 G. Chartas , M. Bautz , G. Garmire , C. Jones , D. P. Schneider

We present a revised strong lensing mass reconstruction of the galaxy cluster RX J1347.5-1145. The X-ray luminous cluster at redshift z=0.451 has already been studied intensively in the past. Based on information of two such previous…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 F. Köhlinger , R. W. Schmidt