Optical-IR SEDs of SDSS quasars in the Spitzer First Look Survey
We analyze the spectral energy distribution (SED) of SDSS-selected quasars in the Spitzer First Look Survey area. Optical+IR colors allow for efficient selection of quasars. We construct a mean quasar SED that can be used to learn about accretion disks, disk-winds, and dusty tori. Future improvements in determining multiwavelength SEDs of different classes of quasars are needed to improve estimates of physical parameters of quasars such as bolometric luminosities and accretion rates.
Additional Information© 2006 Astronomical Society of the Pacific. Funding for the SDSS archive has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, NASA, NSF, the U.S. DoE, the Japanese Monbukagakusho, and the Max Planck Society. Based on archival data obtained with the Spitzer Space Telescope, which is operated by JPL/CalTech under NASA contract 1407. Support for this work was provided by NASA through Contract Number  issued by JPL/Caltech.
Published - 357-0261.pdf