Lyman Break Galaxies at z~3 and Beyond

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dc.creatorSteidel, C. C.
dc.creatorAdelberger, K. L.
dc.creatorDickinson, M.
dc.creatorGiavalisco, M.
dc.creatorPettini, M.
dc.date1998-12-09
dc.date.accessioned2026-07-07T02:29:33Z
dc.date.available2026-07-07T02:29:33Z
dc.descriptionWe report on the status of large surveys of photometrically selected star forming galaxies at z~3 and z~4, with particular emphasis on both the advantages and the limitations of selecting objects using the ``Lyman break'' technique. Current results on the luminosity functions, luminosity densities, color distribution, star formation rates, clustering properties, and the differential evolution of the population as a function of redshift are summarized.
dc.description11 pages, latex; to appear in the proceedings of the Xth Rencontres de Blois, "The Birth of Galaxies", July 1998. Uses blois.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9812167
dc.identifierhttp://arxiv.org/abs/astro-ph/9812167
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13517
dc.subjectAstrophysics
dc.titleLyman Break Galaxies at z~3 and Beyond
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