کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1780329 | 1523804 | 2006 | 4 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Classification and obscuration effects in quasars and galaxies of the CDF-N
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
فیزیک و نجوم
نجوم و فیزیک نجومی
پیش نمایش صفحه اول مقاله
چکیده انگلیسی
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 cmâ2 when we include objects fainter than f0.5-8.0 keV = 3.0 Ã 10â15 erg sâ1 cmâ2. 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.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: New Astronomy Reviews - Volume 50, Issues 9â10, November 2006, Pages 792-795
Journal: New Astronomy Reviews - Volume 50, Issues 9â10, November 2006, Pages 792-795
نویسندگان
Patrick S. Osmer, Stephan Frank,