We present a preliminary investigation of the spectral energy distributions
(SEDs), and star-formation properties of a sample of Mid-IR selected Quasars.
The mid-infrared SEDs of our objects are consistent with that expected from
clumpy torus models. At longer wavelengths, the radio to infrared ratios of
several objects are consistent with those of star-forming galaxies.Comment: Comments: 4 pages, 4 figures. To appear in the proceedings for the
Spitzer Science Center 2005 Conference: Infrared Diagnostics of Galaxy
Evolution, Ed. R. Chary. November, 2005, Pasaden
