SDSS J0903+5028: A New Gravitational Lens
Abstract
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 spectrum showed the presence of a quasar at z= 3.6 in addition to a red galaxy at z=0.388, and the SDSS image showed a second possible quasar image nearby. Follow-up imaging and spectroscopy confirmed the lensing hypothesis. In images taken at the ARC 3.5-meter telescope, two quasars are separated by 2.8 arc-seconds; the lensing galaxy is clearly seen and is blended with one of the quasar images. Spectroscopy taken at the Keck II telescope shows that the quasars have identical redshifts of z=3.6 and both show the presence of the same broad absorption line-like troughs. We present simple lens models which account for the geometry and magnifications. The lens galaxy lies near two groups of galaxies and may be a part of them. The models suggest that the groups may contribute considerable shear and may have a strong effect on the lens configuration.
Cite
@article{arxiv.astro-ph/0307371,
title = {SDSS J0903+5028: A New Gravitational Lens},
author = {David E. Johnston and Gordon T. Richards and Joshua A. Frieman and Charles R. Keeton and Michael A. Strauss and Robert H. Becker and Richard L. White and Eric T. Johnson and Zhaoming Ma and Mark SubbaRao and Neta A. Bahcall and Mariangela Bernardi and Jon Brinkmann and Daniel J. Eisenstein and Masataka Fukugita and Patrick B. Hall and Naohisa Inada and Gillian R. Knapp and Bartosz Pindor and David J. Schlegel and Ryan Scranton and Erin S. Sheldon and Donald P. Schneider and Alexander S. Szalay and Donald G. York},
journal= {arXiv preprint arXiv:astro-ph/0307371},
year = {2009}
}
Comments
submitted to the Astronomical Journal. 27 pages, 7 figures