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Discovery of Two Gravitationally Lensed Quasars with Image Separations of 3″ from the Sloan Digital Sky Survey
Author(s) -
Masamune Oguri,
Naohisa Inada,
Joseph F. Hennawi,
Gordon T. Richards,
David E. Johnston,
Joshua A. Frieman,
B. Pindor,
Michael A. Strauss,
Robert J. Brunner,
R. H. Becker,
F. J. Castander,
Michael D. Gregg,
Patrick B. Hall,
HansWalter Rix,
Donald P. Schneider,
Neta A. Bahcall,
J. Brinkmann,
Donald G. York
Publication year - 2005
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/428087
Subject(s) - quasar , physics , astrophysics , galaxy , sky , redshift , lens (geology) , gravitational lens , cosmology , astronomy , optics
We report the discovery of two doubly-imaged quasars, SDSSJ100128.61+502756.9 and SDSS J120629.65+433217.6, at redshifts of 1.838 and1.789 and with image separations of 2.86'' and 2.90'', respectively. Theobjects were selected as lens candidates from the Sloan Digital Sky Survey(SDSS). Based on the identical nature of the spectra of the two quasars in eachpair and the identification of the lens galaxies, we conclude that the objectsare gravitational lenses. The lenses are complicated; in both systems there areseveral galaxies in the fields very close to the quasars, in addition to thelens galaxies themselves. The lens modeling implies that these nearby galaxiescontribute significantly to the lens potentials. On larger scales, we havedetected an enhancement in the galaxy density near SDSS J100128.61+502756.9.The number of lenses with image separation of ~3'' in the SDSS already exceedsthe prediction of simple theoretical models based on the standardLambda-dominated cosmology and observed velocity function of galaxies.Comment: 24 pages, 9 figures, accepted for publication in Ap

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