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

M.J. Jarvis; S. Rawlings; F.E. Barrio; G.J. Hill; A. Bauer; S. Croft

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

M.J. Jarvis, S. Rawlings, F.E. Barrio, G.J. Hill, A. Bauer, S. Croft

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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.

Original language	English
Title of host publication	In: AGN Physics with the Sloan Digital Sky Survey - ASP Conf Series 311
Publisher	Astronomical Society of the Pacific
Pages	361-4
ISBN (Print)	0-958381-164-8, 978-1-58381-246-4
Publication status	Published - 2004

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title = "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.",

author = "M.J. Jarvis and S. Rawlings and F.E. Barrio and G.J. Hill and A. Bauer and S. Croft",

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year = "2004",

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T1 - A Search for Radio-loud Quasars within the Epoch of Reionization

AU - Jarvis, M.J.

AU - Rawlings, S.

AU - Barrio, F.E.

AU - Hill, G.J.

AU - Bauer, A.

AU - Croft, S.

N1 - Original paper can be found at: http://www.astrosociety.org/pubs/cs/309.html--Copyright Astronomical Society of the Pacific

PY - 2004

Y1 - 2004

N2 - 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.

AB - 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.

M3 - Conference contribution

SN - 0-958381-164-8

SN - 978-1-58381-246-4

SP - 361

EP - 364

BT - In: AGN Physics with the Sloan Digital Sky Survey - ASP Conf Series 311

PB - Astronomical Society of the Pacific

ER -

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

Abstract

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