Bolometric Luminosities and Eddington Ratios of X-Ray Selected Active Galactic Nuclei in the XMM-COSMOS Survey Newer:Spectral Energy Distributions of Type 1 AGN in XMM-COSMOS Survey II - Shape EvolutionOlder:Evolution of the Quasar Luminosity Function over 3 < z < 5 in the COSMOS Survey Field PostedSeptember 1, 2012 AuthorScienceSites Categories2012