{ "id": "1809.07337", "version": "v1", "published": "2018-09-19T18:00:02.000Z", "updated": "2018-09-19T18:00:02.000Z", "title": "SDSS J0909$+$4449: A Large-separation Strongly Lensed Quasar at $z \\sim 2.8$ with Three Images", "authors": [ "Yiping Shu", "Rui Marques-Chaves", "N. Wyn Evans", "Ismael Pérez-Fournon" ], "comment": "5 pages, 3 figures, accepted for publication in the MNRAS Letter", "categories": [ "astro-ph.GA" ], "abstract": "We report the discovery of SDSS J0909$+$4449, an exceptional system consisting of a quasar at $z=2.788$ strongly lensed by a group of galaxies at $z \\sim 0.9$ into three images separated by up to 14\\arcsec\\, based on archival data collected by the Sloan Digital Sky Survey, extended Baryon Oscillation Spectroscopic Survey, Beijing--Arizona Sky Survey, the Mayall z-band Legacy Survey, and the Gemini Telescope. We discuss two hypotheses on the nature of SDSS J0909$+$4449, i.e. a rare triply-imaged quasar in the naked cusp configuration and a typical quadruply-imaged quasar with the fourth image undetected in the current data. We find that simple lens models can provide excellent fits to the observed image positions and the non-detection under either hypothesis. Deeper imaging data, spectroscopic observations, and follow-up light curve measurements will be helpful in determining which hypothesis is correct and provide better constraints on the lens mass distribution. Nevertheless, given its unusually large image separations, SDSS J0909$+$4449 will be a unique probe for the mass structure and the underlying cooling and stellar feedback processes on group or cluster scales.", "revisions": [ { "version": "v1", "updated": "2018-09-19T18:00:02.000Z" } ], "analyses": { "keywords": [ "large-separation strongly lensed quasar", "sdss j0909", "extended baryon oscillation spectroscopic survey", "mayall z-band legacy survey", "sloan digital sky survey" ], "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable" } } }