{ "id": "1505.05273", "version": "v1", "published": "2015-05-20T08:09:04.000Z", "updated": "2015-05-20T08:09:04.000Z", "title": "Herschel Survey of the Palomar-Green QSOs at Low Redshift", "authors": [ "Andreea O. Petric", "Luis C. Ho", "Nicolas J. M. Flagey", "Nicholas Z. Scoville" ], "comment": "accepted for publication in ApJS", "categories": [ "astro-ph.GA" ], "abstract": "We investigate the global cold dust properties of 85 nearby (z < 0.5) QSOs, chosen from the Palomar-Green sample of optically luminous quasars. We determine their infrared spectral energy distributions and estimate their rest-frame luminosities by combining Herschel data from 70 to 500 microns with near-infrared and mid-infrared measurements from the Two Micron All Sky Survey (2MASS) and the Wide-Field Infrared Survey Explorer (WISE). In most sources the far-infrared (FIR) emission can be attributed to thermally heated dust. Single temperature modified black body fits to the FIR photometry give an average dust temperature for the sample of 33~K, with a standard deviation of 8~K, and an average dust mass of 7E6 Solar Masses with a standard deviation of 9E6 Solar Masses. Estimates of star-formation that are based on the FIR continuum emission correlate with those based on the 11.3 microns PAH feature, however, the star-formation rates estimated from the FIR continuum are higher than those estimated from the 11.3 microns PAH emission. We attribute this result to a variety of factors including the possible destruction of the PAHs and that, in some sources, a fraction of the FIR originates from dust heated by the active galactic nucleus and by old stars.", "revisions": [ { "version": "v1", "updated": "2015-05-20T08:09:04.000Z" } ], "analyses": { "keywords": [ "herschel survey", "palomar-green qsos", "low redshift", "temperature modified black body fits", "standard deviation" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }