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Evolution of optically faint AGN from COMBO-17 and GEMS

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arxiv astro-ph/0404331 v1 pith:6PHL6SNM submitted 2004-04-16 astro-ph

Evolution of optically faint AGN from COMBO-17 and GEMS

L. Wisotzki , K. Jahnke , S.F. Sanchez , C. Wolf , M. Barden , E.F. Bell , A. Borch , B. HaeUssler
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K. Meisenheimer H.-W. Rix S.V.W. Beckwith J.A.R. Caldwell S. Jogee R.S. Somerville D.H. McIntosh C.Y. Peng (the GEMS collaboration)
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keywords evolutiongemsanalysedapparentassesschandracombo-17cosmic
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We have mapped the AGN luminosity function and its evolution between z=1 and z=5 down to apparent magnitudes of $R<24$. Within the GEMS project we have analysed HST-ACS images of many AGN in the Extended Chandra Deep Field South, enabling us to assess the evolution of AGN host galaxy properties with cosmic time.

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