{ "id": "0801.3729", "version": "v1", "published": "2008-01-24T10:49:37.000Z", "updated": "2008-01-24T10:49:37.000Z", "title": "Optical monitoring of the z=4.40 quasar Q 2203+292", "authors": [ "E. P. Ovcharov", "P. L. Nedialkov", "A. T. Valcheva", "V. D. Ivanov", "N. A. Tikhonov", "I. S. Stanev", "A. B. Kostov", "Ts. B. Georgiev" ], "comment": "9 pages, 8 figures, accepted for publication in MNRAS", "doi": "10.1111/j.1365-2966.2008.12990.x", "categories": [ "astro-ph" ], "abstract": "We report Cousins R-band monitoring of the high-redshift (z=4.40) radio quiet quasar Q 2203+292 from May 1999 to October 2007. The quasar shows maximum peak-to-peak light curve amplitude of ~0.3 mag during the time of our monitoring, and ~0.9 mag when combined with older literature data. The rms of a fit to the light curve with a constant is 0.08 mag and 0.2 mag, respectively. The detected changes are at ~3-sigma level. The quasar was in a stable state during the recent years and it might have undergone a brightening event in the past. The structure function analysis concluded that the object shows variability properties similar to those of the lower redshift quasars. We set a lower limit to the Q 2203+292 broad line region mass of 0.3-0.4 M_odot. Narrow-band imaging search for redshifted Ly_alpha from other emission line objects at the same redshift shows no emission line objects in the quasar vicinity.", "revisions": [ { "version": "v1", "updated": "2008-01-24T10:49:37.000Z" } ], "analyses": { "keywords": [ "emission line objects", "optical monitoring", "maximum peak-to-peak light curve amplitude", "broad line region mass", "structure function analysis" ], "tags": [ "journal article" ], "publication": { "publisher": "Wiley-Blackwell", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2008, "month": "May", "volume": 386, "number": 2, "pages": 819 }, "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable", "inspire": 778060, "adsabs": "2008MNRAS.386..819O" } } }