Mass Models and Environment of the New Quadruply Lensed Quasar SDSS J1330+1810 [electronic resource]

Astrophysics,Astro, Grqc.

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Bibliographic Details
Online Access: Online Access
Corporate Author: Stanford Linear Accelerator Center (Researcher)
Format: Government Document Electronic eBook
Language:English
Published: Washington, D.C. : Oak Ridge, Tenn. : United States. Department of Energy. ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, 2008.
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Summary:Astrophysics,Astro, Grqc.
Abstract:We present the discovery of a new quadruply lensed quasar. The lens system, SDSS J1330+1810 at z{sub s} = 1.393, was identified as a lens candidate from the spectroscopic sample of the Sloan Digital Sky Survey. Optical and near-infrared images clearly show four quasar images with a maximum image separation of 1.76 inch, as well as a bright lensing galaxy. We measure a redshift of the lensing galaxy of zā‚ = 0.373 from absorption features in the spectrum. We find a foreground group of galaxies at z = 0.31 centred ā‰ˆ 120 inch southwest of the lens system. Simple mass models fit the data quite well, including the flux ratios between images, although the lens galaxy appears to be ā‰ˆ 1 mag brighter than expected by the Faber-Jackson relation. Our mass modeling suggests that shear from nearby structure is affecting the lens potential.
Item Description:Published through SciTech Connect.
09/09/2008.
"slac-pub-13382"
"arXiv:0809.0913"
Monthly Notices of the Royal Astronomical Society ISSN 0035-8711; MNRAA4 FT.
Inada, Naohisa; Oguri, Masamune; Kayo, Issha; Shin, Min-Su; Schneider, Donald P.; Strauss, Michael A.; York, Donald G.; Blackburne, Jeffrey A.
Physical Description:9 pages : digital, PDF file.