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

dc.creatorJarvis, Matt J.
dc.creatorRawlings, Steve
dc.creatorBarrio, F. Eugenio
dc.creatorHill, Gary J.
dc.creatorBauer, Amanda
dc.creatorCroft, Steve
dc.date2003-09-15
dc.date.accessioned2026-07-07T02:09:34Z
dc.date.available2026-07-07T02:09:34Z
dc.descriptionThe 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.
dc.description4 pages, 1 figure. To appear in "AGN Physics with the Sloan Digital Sky Survey, ed. G. T. Richards and P. B. Hall (San Francisco: ASP)"
dc.identifierhttps://arxiv.org/abs/astro-ph/0309379
dc.identifierhttp://arxiv.org/abs/astro-ph/0309379
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6476
dc.subjectAstrophysics
dc.titleA Search for Radio-loud Quasars within the Epoch of Reionization
dc.typetext

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