Classification and obscuration effects in quasars and galaxies of the CDF-N

✍ Scribed by Patrick S. Osmer; Stephan Frank

• Publisher: Elsevier Science
• Year: 2006
• Tongue: English
• Weight: 303 KB
• Volume: 50
• Category: Article
• ISSN: 1387-6473
• DOI: 10.1016/j.newar.2006.06.075

✦ Synopsis

We present a classification scheme for Chandra Deep Field-North (CDF-N) sources with spectroscopic redshifts based upon their broadband spectral energy distributions. A substantial fraction of the faint sources can be identified as normal/star-forming galaxies. The AGN in the sample divide into four classes: luminous, apparently unabsorbed QSOs; objects with reddened optical spectra and no signs of X-ray absorption; apparently X-ray absorbed AGN with no signs of reddening in their optical spectra; and optically reddened sources with X-ray spectra indicative of substantial obscuration. The observed column density distribution for the complete sample shows a significant rise of the number of sources with N H > 10 22.5 cm À2 when we include objects fainter than f 0.5-8.0 keV = 3.0 • 10 À15 erg s À1 cm À2 . Our results indicate that a full X-ray spectral analysis of the complete sample is crucial in mapping out the underlying absorbing column density distribution, and thus the effects of obscuration on the number counts and luminosity functions.