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相关论文: An initial analysis of a strongly-lensed QSOs cand…

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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 report the discovery of a new gravitational lens candidate Q2138-431AB, comprising two quasar images at a redshift of 1.641 separated by 4.5 arcsecs. The spectra of the two images are very similar, and the redshifts agree to better than…

天体物理学 · 物理学 2016-08-15 M. R. S. Hawkins , D. Clements , J. W. Fried , A. F. Heavens , P. Véron , E. M. Minty , P. van der Werf

This paper reviews the question of whether the wide separation double quasar Q2138-431 is a gravitational lens. From early work, the two quasar images are known to have almost identical spectra and redshifts, but no lensing galaxy has so…

星系天体物理 · 物理学 2021-04-16 M. R. S. Hawkins

We present the first lensing total mass estimate of a galaxy, at redshift 2.207, that acts as a gravitational deflector and damped Lyman-alpha absorber on the background QSO SDSS J1135-0010, at redshift 2.888. The remarkably small projected…

宇宙学与河外天体物理 · 物理学 2015-06-18 C. Grillo , J. P. U. Fynbo

The gravitational lens system CLASS B2108+213 has two radio-loud lensed images separated by 4.56 arcsec. The relatively large image separation implies that the lensing is caused by a group of galaxies. In this paper, new optical imaging and…

宇宙学与河外天体物理 · 物理学 2015-05-14 J. P. McKean , M. W. Auger , L. V. E. Koopmans , S. Vegetti , O. Czoske , C. D. Fassnacht , T. Treu , A. More , D. D. Kocevski

We report the discovery of a new gravitationally lensed QSO, at a redshift z = 1.689, with four QSO components in a cross-shaped arrangement around a bright galaxy. The maximum separation between images is 2.6 arcsec, enabling a reliable…

天体物理学 · 物理学 2009-11-07 Lutz Wisotzki , Paul L. Schechter , Hale V. Bradt , Janine Heinmueller , Dieter Reimers

Gravitational lens modeling is presented for the first discovered example of a three-component source for which each component is quadruply imaged. The lens is a massive galaxy member of the cluster Cl J0152.7-1357 at z ~ 0.84. Taking…

天体物理学 · 物理学 2009-11-13 C. Grillo , M. Lombardi , P. Rosati , G. Bertin , R. Gobat , R. Demarco , C. Lidman , V. Motta , M. Nonino

We present a detailed strong lensing analysis of an HST/ACS legacy dataset for the first gravitational lens, Q0957+561. With deep imaging we identify 24 new strongly lensed features, which we use to constrain mass models. We model the…

宇宙学与河外天体物理 · 物理学 2014-11-20 Ross Fadely , Charles R. Keeton , Reiko Nakajima , Gary M. Bernstein

We report the discovery of a new quadruply imaged quasar surrounded by an optical Einstein ring candidate. Spectra of the different components of 1RXS J113155.4-123155 reveal a source at z=0.658. Up to now, this object is the closest known…

天体物理学 · 物理学 2009-11-10 D. Sluse , J. Surdej , J. -F. Claeskens , D. Hutsemekers , C. Jean , F. Courbin , T. Nakos , M. Billeres , S. V. Khmil

We report the discovery of the new gravitational lens system HE~0230$-$2130, a QSO at redshift $z=2.162$ consisting of at least five distinct components. Three of these are clearly lensed images of the QSO, one is most likely the lensing…

天体物理学 · 物理学 2007-05-23 L. Wisotzki , N. Christlieb , M. C. Liu , J. Maza , N. D. Morgan , P. L. Schechter

We report the serendipitous discovery of an "Einstein Ring" in the optical band from the Sloan Digital Sky Survey (SDSS) data and associated four images of a background source. The lens galaxy appears to be a nearby dwarf spheroid at a…

天体物理学 · 物理学 2011-02-11 Kajal K Ghosh , D. Narasimha

[abridged] We present VLT/FORS1 spectroscopic follow-up observations and HST/WFPC2 imaging of the system COSMOS 5921+0638, which exhibits quadruply lensed images and a perfect Einstein ring. We investigate the nature of COSMOS 5921+0638 by…

宇宙学与河外天体物理 · 物理学 2009-11-19 T. Anguita , C. Faure , J. -P. Kneib , J. Wambsganss , C. Knobel , A. M. Koekemoer , M. Limousin

The large-redshift (z=3.8) quasar 1208+1011 has recently been discovered to be a gravitational lens candidate with a separation of 0.47" between the two imaged components (A and B). NOT (Nordic Optical Telescope) and HST (Hubble Space…

天体物理学 · 物理学 2011-05-23 Jens Hjorth , Frank Grundahl , Kari Nilsson , Leif Festin

We present the first case of strong gravitational lensing by a QSO : SDSS J0013+1523, at z = 0.120. The discovery is the result of a systematic search for emission lines redshifted behind QSOs, among 22298 spectra of the SDSS data release…

宇宙学与河外天体物理 · 物理学 2010-08-09 F. Courbin , M. Tewes , S. G. Djorgovski , D. Sluse , A. Mahabal , F. Rerat , G. Meylan

We present spectroscopic confirmation of two new lensed quasars via data obtained at the 6.5m Magellan/Baade Telescope. The lens candidates have been selected from the Dark Energy Survey (DES) and WISE based on their multi-band photometry…

We model the mass distribution in the recently discovered Einstein ring LBG J213512.73-010143 (the `Cosmic Eye') using archival Hubble Space Telescope imaging. We reconstruct the mass density profile of the z=0.73 lens and the surface…

天体物理学 · 物理学 2009-06-23 Simon Dye , Ian Smail , A. M. Swinbank , H. Ebeling , A. C. Edge

We present a sample of 12 Quasi-Stellar Objects (QSOs) potentially acting as strong gravitational lenses on background Emission Line Galaxies (ELG) or Lyman-$\alpha$ Emitters (LAEs) selected selected through a systematic search of the…

星系天体物理 · 物理学 2019-05-13 Romain A. Meyer , Timothée Delubac , Jean-Paul Kneib , Frédéric Courbin

We analyze a new gravitational lens, OAC-GL J1223-1239, serendipitously found in a deep I-band image of the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS). The lens is a L_*, edge-on S0 galaxy at z=0.4656. The gravitational…

The quasar HE 0047-1756, at z=1.67, is found to be split into two images 1.44" apart by an intervening galaxy acting as a gravitational lens. The flux ratio for the two components is roughly 3.5:1, depending slightly upon wavelength. The…

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