1209.1478 (M. Elvis et al.)

Spectral Energy Distributions of Type 1 AGN in the COSMOS Survey I - The XMM-COSMOS Sample    [PDF]

M. Elvis, H. Hao, F. Civano, M. Brusa, M. Salvato, A. Bongiorno, P. Capak, G. Zamorani, A. Comastri, K. Jahnke, E. Lusso, V. Mainieri, J. R. Trump, L. Ho, H. Aussel, N. Cappelluti, M. Cisternas, D. Frayer, R. Gilli, G. Hasinger, J. P. Huchra, C. D. Impey, A. M. Koekemoer, G. Lanzuisi, E. Le Floc'h, S. J. Lilly, Y. Liu, P. McCarthy, H. J. McCracken, A. Merloni, H. J. Roeser, D. B. Sanders, M. Sargent, N. Scoville, E. Schinnerer, D. Schiminovich, J. Silverman, Y. Taniguchi, C. Vignali, C. M. Urry, M. A. Zamojski, M. Zatloukal

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.

View original: http://arxiv.org/abs/1209.1478