Spectral Energy Distributions of Type 1 AGN in the COSMOS Survey I - The
  XMM-COSMOS Sample
  The "Cosmic Evolution Survey" (COSMOS) enables the study of the Spectral
Energy Distributions (SEDs) of Active Galactic Nuclei (AGN) because of the deep
coverage and rich sampling of frequencies from X-ray to radio. Here we present
a SED catalog of 413 X-ray (\xmm) selected type 1 (emission line FWHM$>2000$ km
s$^{-1}$) AGN with Magellan, SDSS or VLT spectrum. The SEDs are corrected for
the Galactic extinction, for broad emission line contributions, constrained
variability, and for host galaxy contribution. We present the mean SED and the
dispersion SEDs after the above corrections in the rest frame 1.4 GHz to 40
keV, and show examples of the variety of SEDs encountered. In the near-infrared
to optical (rest frame $\sim 8\mu m$-- 4000\AA), the photometry is complete for
the whole sample and the mean SED is derived from detections only. Reddening
and host galaxy contamination could account for a large fraction of the
observed SED variety. The SEDs are all available on-line.
