Spitzer/IRS Spectra of GOODS AGN

Details Spitzer/IRS Spectra of GOODS AGN Spitzer/IRS Spectra of GOODS AGN

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.5207v&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #52.07; Bulletin of the American Astronomical Society, V

Astronomy and Astrophysics

Astronomy

Scientific paper

IRS Spectra of GOODS AGN
Infrared emission from AGN comes from dust heated by black hole accretion and/or star-formation. Separating the contributions in optical/UV light can be difficult, particularly when obscuration is high; mid-infrared spectra are less affected by obscuration and thus offer diagnostics of the underlying power source(s). We present Spitzer IRS spectra of 10 IR-bright, hard X-ray-selected AGN from the GOODS-North field, spanning the redshift range 0.485This work was supported by NASA JPL/Spitzer grant RSA 177278. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA JPL/Spitzer grant RSA 177278.

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