Lyman Break Galaxies at z 3 and Beyond
Steidel, C. C. · Adelberger, K. L. · Dickinson, M. · Giavalisco, M. · Pettini, M.
Original · EN
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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