A large area search for radio-loud quasars within the epoch of reionization
The Universe became fully reionized, and observable optically, at a time corresponding to redshift z ~ 6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that one can hope to make detailed studies of the earliest stages of galaxy formatio...
| Main Authors: | , , , , , |
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| Other Authors: | |
| Format: | Conference item |
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World Scientific Publishing Co. Pte. Ltd.
2004
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| _version_ | 1826289584507453440 |
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| author | Jarvis, M Rawlings, S Barrio, F Hill, G Bauer, A Croft, S |
| author2 | Mújica, R |
| author_facet | Mújica, R Jarvis, M Rawlings, S Barrio, F Hill, G Bauer, A Croft, S |
| author_sort | Jarvis, M |
| collection | OXFORD |
| description | The Universe became fully reionized, and observable optically, at a time corresponding to redshift z ~ 6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that one can hope to make detailed studies of the earliest stages of galaxy formation. At present no targets for such studies are known. In these proceedings we describe a survey which is underway to find radio-loud quasars at z > 6.5, and present broad-band SEDs of our most promising candidates. |
| first_indexed | 2024-03-07T02:31:07Z |
| format | Conference item |
| id | oxford-uuid:a744b7e4-0e82-44f1-964d-7959094595f8 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T02:31:07Z |
| publishDate | 2004 |
| publisher | World Scientific Publishing Co. Pte. Ltd. |
| record_format | dspace |
| spelling | oxford-uuid:a744b7e4-0e82-44f1-964d-7959094595f82022-03-27T02:53:24ZA large area search for radio-loud quasars within the epoch of reionizationConference itemhttp://purl.org/coar/resource_type/c_5794uuid:a744b7e4-0e82-44f1-964d-7959094595f8Symplectic Elements at OxfordWorld Scientific Publishing Co. Pte. Ltd.2004Jarvis, MRawlings, SBarrio, FHill, GBauer, ACroft, SMújica, RMaiolino, RThe Universe became fully reionized, and observable optically, at a time corresponding to redshift z ~ 6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that one can hope to make detailed studies of the earliest stages of galaxy formation. At present no targets for such studies are known. In these proceedings we describe a survey which is underway to find radio-loud quasars at z > 6.5, and present broad-band SEDs of our most promising candidates. |
| spellingShingle | Jarvis, M Rawlings, S Barrio, F Hill, G Bauer, A Croft, S A large area search for radio-loud quasars within the epoch of reionization |
| title | A large area search for radio-loud quasars within the epoch of reionization |
| title_full | A large area search for radio-loud quasars within the epoch of reionization |
| title_fullStr | A large area search for radio-loud quasars within the epoch of reionization |
| title_full_unstemmed | A large area search for radio-loud quasars within the epoch of reionization |
| title_short | A large area search for radio-loud quasars within the epoch of reionization |
| title_sort | large area search for radio loud quasars within the epoch of reionization |
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