The XMM-Newton Wide-field Survey in the Cosmos Field (XMM-COSMOS): Demography and Multiwavelength Properties of Obscured and Unobscured Luminous Active Galactic Nuclei Newer:Ultraluminous X-Ray Sources Out to z ~ 0.3 in the COSMOS FieldOlder:Detailed Decomposition of Galaxy Images. II. Beyond Axisymmetric Models PostedMay 18, 2010 AuthorScienceSites Categories2010