Discovery of Four Gravitationally Lensed Quasars from the Sloan Digital Sky Survey
| dc.creator | Oguri, Masamune | |
| dc.creator | Inada, Naohisa | |
| dc.creator | Clocchiatti, Alejandro | |
| dc.creator | Kayo, Issha | |
| dc.creator | Shin, Min-Su | |
| dc.creator | Hennawi, Joseph F. | |
| dc.creator | Strauss, Michael A. | |
| dc.creator | Morokuma, Tomoki | |
| dc.creator | Schneider, Donald P. | |
| dc.creator | York, Donald G. | |
| dc.date | 2007-08-07 | |
| dc.date | 2007-11-25 | |
| dc.date.accessioned | 2026-07-07T11:41:43Z | |
| dc.date.available | 2026-07-07T11:41:43Z | |
| dc.description | We present the discovery of four gravitationally lensed quasars selected from the spectroscopic quasar catalog of the Sloan Digital Sky Survey. We describe imaging and spectroscopic follow-up observations that support the lensing interpretation of the following four quasars: SDSS J0832+0404 (image separation θ=1.98", source redshift z_s=1.115, lens redshift z_l=0.659); SDSS J1216+3529 (θ=1.49", z_s=2.012); SDSS J1322+1052 (θ=2.00", z_s=1.716); and SDSS J1524+4409 (θ=1.67", z_s=1.210, z_l=0.320). Each system has two lensed images. We find that the fainter image component of SDSS J0832+0404 is significantly redder than the brighter component, perhaps because of differential reddening by the lensing galaxy. The lens potential of SDSS J1216+3529 might be complicated by the presence of a secondary galaxy near the main lensing galaxy. | |
| dc.description | 25 pages, 10 figures, 6 tables, accepted for publication in AJ | |
| dc.identifier | https://arxiv.org/abs/0708.0871 | |
| dc.identifier | http://arxiv.org/abs/0708.0871 | |
| dc.identifier | Astron.J.135:520-526,2008 | |
| dc.identifier | doi:10.1088/0004-6256/135/2/520 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/200636 | |
| dc.subject | Astrophysics | |
| dc.title | Discovery of Four Gravitationally Lensed Quasars from the Sloan Digital Sky Survey | |
| dc.type | text |