We derive the properties of dusty tori in active galactic nuclei from the comparison of observed spectral energy distributions (SEDs) of SDSS quasars and a precomputed grid of torus models. The observed SEDs comprise SDSS photometry, Two-Micron All-Sky Survey J, H and K data, whenever available, and mid-infrared (mid-IR) data from the Spitzer Wide-area InfraRed Extragalactic Survey.
Cone search capability for table J/MNRAS/386/1252/qsos (Coordinates, redshifts, SDSS photometry, 2MASS photometry, IRAC and MIPS 24{mu}m fluxes for the SWIRE/SDSS quasars)