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25 April 2024 |
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Article overview
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X-ray emitting AGN unveiled by the Chandra Multiwavelength Project | John D. Silverman
; Paul J. Green
; Thomas L. Aldcroft
; Dong-Woo Kim
; Wayne Barkhouse
; Robert A. Cameron
; Belinda J. Wilkes
; | Date: |
31 Oct 2003 | Subject: | astro-ph | Affiliation: | Harvard-Smithsonian Center for Astrophysics | Abstract: | We present an X-ray and optical analysis of a 2-8 keV flux limited (fx > 10e-14 erg s^-1 cm^-2) sample of 126 AGN detected in 16 Chandra fields. This work represents a small though significant subset of the Chandra Multiwavelength Project (ChaMP). We have chosen this limiting flux to have a reasonable degree of completeness (50%) in our optical spectroscopic identifications. The optical counterparts of these AGN are characterized as either broad emission line AGN (BLAGN; 67%), narrow emission line galaxies (NELG; 22%) or absorption line galaxies (ALG; 11%) without any evidence of an AGN signature. Based on their X-ray luminosity and spectral properties, we show that NELG and ALG are primarily the hosts of obscured AGN with an intrinsic absorbing column in the range of 10^21.5 | Source: | arXiv, astro-ph/0310907 | Services: | Forum | Review | PDF | Favorites |
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