Evolution of optically faint AGN from COMBO-17 and GEMS
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 properti...
| Main Authors: | , , , , , , , , , , , , , , , |
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| Format: | Journal article |
| Published: |
2004
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| _version_ | 1797091893118500864 |
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| author | Wisotzki, L Jahnke, K Sanchez, S Wolf, C Barden, M Bell, E Borch, A HaeUssler, B Meisenheimer, K Rix, H Beckwith, S Caldwell, J Jogee, S Somerville, R McIntosh, D Peng, C |
| author_facet | Wisotzki, L Jahnke, K Sanchez, S Wolf, C Barden, M Bell, E Borch, A HaeUssler, B Meisenheimer, K Rix, H Beckwith, S Caldwell, J Jogee, S Somerville, R McIntosh, D Peng, C |
| author_sort | Wisotzki, L |
| collection | OXFORD |
| description | 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. |
| first_indexed | 2024-03-07T03:38:52Z |
| format | Journal article |
| id | oxford-uuid:bd35eba4-ebae-4991-97cf-5f83a6f1f822 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T03:38:52Z |
| publishDate | 2004 |
| record_format | dspace |
| spelling | oxford-uuid:bd35eba4-ebae-4991-97cf-5f83a6f1f8222022-03-27T05:30:04ZEvolution of optically faint AGN from COMBO-17 and GEMSJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:bd35eba4-ebae-4991-97cf-5f83a6f1f822Symplectic Elements at Oxford2004Wisotzki, LJahnke, KSanchez, SWolf, CBarden, MBell, EBorch, AHaeUssler, BMeisenheimer, KRix, HBeckwith, SCaldwell, JJogee, SSomerville, RMcIntosh, DPeng, CWe 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. |
| spellingShingle | Wisotzki, L Jahnke, K Sanchez, S Wolf, C Barden, M Bell, E Borch, A HaeUssler, B Meisenheimer, K Rix, H Beckwith, S Caldwell, J Jogee, S Somerville, R McIntosh, D Peng, C Evolution of optically faint AGN from COMBO-17 and GEMS |
| title | Evolution of optically faint AGN from COMBO-17 and GEMS |
| title_full | Evolution of optically faint AGN from COMBO-17 and GEMS |
| title_fullStr | Evolution of optically faint AGN from COMBO-17 and GEMS |
| title_full_unstemmed | Evolution of optically faint AGN from COMBO-17 and GEMS |
| title_short | Evolution of optically faint AGN from COMBO-17 and GEMS |
| title_sort | evolution of optically faint agn from combo 17 and gems |
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