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20 April 2024 |
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Infrared Properties of AGN in the GOODS Fields: AGN in Stellar Dominated High-z Galaxies | | Jeffrey Van Duyne
; C. Meg Urry
; Eleni Chatzichristou
; Ezequiel Treister the GOODS AGN Team
; | | Date: |
2 Mar 2005 | | Subject: | astro-ph | | Affiliation: | 1,2), Eleni Chatzichristou , Ezequiel Treister (1,3) the GOODS AGN Team, ( Astronomy Dept., Yale U., Physics Dept., Yale U., Depto de Astronomia, U. de Chile | | Abstract: | We present analysis of spectral energy distributions (SEDs) from mid-infrared through X-ray of a sample of 420 hard X-ray selected, z-band and Spitzer/IRAC detected active galactic nuclei (AGN) and AGN candidates from the GOODS multiwavelength survey. We fit local empirical SED templates of both normal and active galaxies to the rest-frame luminosities calculated from spectroscopic (where available) and photometric redshifts. The majority of the optically stellar-dominated (with early-type galaxy fits) sources are moderately luminous (L_X,2-10 keV ~ 10^43 erg/s) hard X-ray sources with high X-ray hardness ratios (HR > 0.2), high MIR luminosities and red MIR colors in excess of a typical stellar dominated elliptical galaxy. These sources likely harbor heavily obscured (though Compton-thin) AGN. The observed ratio of obscured to unobscured AGN has an integrated mean of ~3.4:1 but declines with increasing redshift. This effect has been explained by Treister et al. (2004) as an observational bias triggered by the lack of spectroscopic redshifts at R > 24 which are predominantly higher redshift obscured sources. | | Source: | arXiv, astro-ph/0503056 | | Services: | Forum | Review | PDF | Favorites | |
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