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Lyman Break Galaxies at z~3 and Beyond

1998/12/09 by C. C. Steidel, Steidel, C. C., K. L. Adelberger +7
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9812167

11 pages, latex; to appear in the proceedings of the Xth Rencontres de Blois, "The Birth of Galaxies", July 1998. Uses blois.sty

arxiv created 1998/12/09 · arxiv updated 2009/12/01

Abstract

We 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.

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