- Abstract:
- 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.
- Publication status:
- Published
- Version:
- Accepted Manuscript
- Files:
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(pdf, 132.7kb)
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- Publisher copy:
- 10.1142/9789812702432_0034
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- Publisher:
- World Scientific Publishing Co. Pte. Ltd. Publisher's website
- Pages:
- 133–136
- Publication date:
- 2004-10-05
- DOI:
- URN:
-
uuid:a744b7e4-0e82-44f1-964d-7959094595f8
- Source identifiers:
-
10666
- Local pid:
- pubs:10666
- ISBN:
- 981-256-049-1
- Keywords:
- Copyright holder:
- World Scientific Publishing Co. Pte. Ltd.
- Copyright date:
- 2004
- Notes:
-
adsurl: http://adsabs.harvard.edu/abs/2004mas..conf..133J
adsnote: Provided by the SAO/NASA Astrophysics Data System
Electronic version of an article published as Multiwavelength AGN Surveys, 2004, 133–136, http://dx.doi.org/10.1142/9789812702432_0034. Copyright © 2004 by World Scientific Publishing Co. Pte. Ltd. http://www.worldscientific.com/doi/abs/10.1142/9789812702432_0034
Conference
A large area search for radio-loud quasars within the epoch of reionization
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