Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006newar..50..792o&link_type=abstract
New Astronomy Reviews, Volume 50, Issue 9-10, p. 792-795.
Astronomy and Astrophysics
Astronomy
Scientific paper
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 NH > 1022.5 cm-2 when we include objects fainter than f0.5 8.0 keV = 3.0 × 10-15 erg s-1 cm-2. 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.
Frank Stephan
Osmer Patrick S.
No associations
LandOfFree
Classification and obscuration effects in quasars and galaxies of the CDF-N does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Classification and obscuration effects in quasars and galaxies of the CDF-N, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Classification and obscuration effects in quasars and galaxies of the CDF-N will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1344263