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A Search for Radio-loud Quasars within the Epoch of Reionization

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.
Publication status:
Published

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author

Contributors

Role:
Editor
Role:
Editor
Publisher:
Astronomical Society of the Pacific Publisher's website
Host title:
AGN Physics with the Sloan Digital Sky Survey
Series:
Astronomical Society of the Pacific conference series
Volume:
311
Pages:
361-364
Publication date:
2004-06-01
ISBN:
1583811648
Keywords:
Pubs id:
pubs:23837
UUID:
uuid:6866f36e-d945-4a25-a53d-74f090133aec
Local pid:
pubs:23837
Source identifiers:
23837
Deposit date:
2012-12-19

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