Evolution of Optically Faint AGN from the COMBO-17 and GEMS
Wisotzki, L.; Jahnke, K.; Sanchez, S. F.; Wolf, C.;Barden, M.; Bell, E. F.; Borch, A.; Häussler, B.;Meisenheimer, K.; Rix, H.-W.; Beckwith, S. V. W.;Caldwell, J. A. R.; Jogee, S.; Somerville, R. S.;McIntosh, D. H.; Peng, C. Y.. Evolution of Optically Faint AGN from the COMBO-17 and GEMS. Multiwavelength AGN Surveys; proceedings of the Guillermo Haro Conference held December 8-12, 2003, in Cozumel, Mexico. Edited by Raúl Mújica and Roberto Maiolino. ISBN 981-256-049-1. Published by World Scientific Publishing Company, Singapore, 2004, p.63. 2004, Vol. , p. -2004.
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.
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.