Evolution of the Quasar Luminosity Function over 3 < z < 5 in the COSMOS Survey Field Newer:Bolometric Luminosities and Eddington Ratios of X-Ray Selected Active Galactic Nuclei in the XMM-COSMOS SurveyOlder:The Chandra COSMOS Survey PostedAugust 7, 2012 AuthorScienceSites Categories2012