2006/09/26 by Tomoki Morokuma, Naohisa Inada, Masamune Oguri +11 · 31 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gravitational lens #Lens (geology) #Luminosity #Optics #Physics #Quasar #Sky #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/509701
published in The Astronomical Journal 133(1), 214-219 (Institute of Physics) · 16 pages, 4 figures, the Astronomical Journal accepted
arxiv created 2006/09/26 · openalex publication_date 2006/12/11 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
We report the discovery of the two-image gravitationally lensed quasar SDSS J133222.62+034739.9 (SDSS J1332+0347) with an image separation of Δθ = 1.14''. This system consists of a source quasar at z s = 1.445 and a lens galaxy at z l = 0.191. The agreement of the luminosity, ellipticity, and position angle of the lens galaxy with those expected from a lens model confirms the lensing hypothesis.