{ "id": "1608.00465", "version": "v1", "published": "2016-08-01T15:13:34.000Z", "updated": "2016-08-01T15:13:34.000Z", "title": "The Mid-Infrared Luminosity Evolution and Luminosity Function of Quasars with SDSS and WISE", "authors": [ "J. Singal", "J. George", "A. Gerber" ], "comment": "13 pages, 11 figures, submitted to ApJ. arXiv admin note: text overlap with arXiv:1207.3396", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "We determine the 22$\\mu$m luminosity evolution and luminosity function for quasars from a data set of over 20,000 objects obtained by combining flux-limited Sloan Digital Sky Survey optical and Wide field Infrared Survey Explorer mid-infrared data. We apply methods developed in previous works to access the intrinsic population distributions non-parametrically, taking into account the truncations and correlations inherent in the data. We find that the population of quasars exhibits positive luminosity evolution with redshift in the mid-infrared, but with considerably less mid-infrared evolution than in the optical or radio bands. With the luminosity evolutions accounted for, we determine the density evolution and local mid-infrared luminosity function. The latter displays a sharp flattening at local luminosities below $\\sim 10^{31}$ erg sec$^{-1}$ Hz$^{-1}$, which has been reported previously at 15 $\\mu$m for AGN classified as both type-1 and type-2. We calculate the integrated total emission from quasars at 22 $\\mu$m and find it to be a small fraction of both the cosmic infrared background light and the integrated emission from all sources at this wavelength.", "revisions": [ { "version": "v1", "updated": "2016-08-01T15:13:34.000Z" } ], "analyses": { "keywords": [ "luminosity function", "mid-infrared luminosity evolution", "sloan digital sky survey", "survey explorer mid-infrared data", "field infrared survey explorer" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }