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Keck Deep Fields. II. The UV Galaxy Luminosity Function at z~4, 3, and 2
ASTROPHYSICAL JOURNAL, no. 2 (2006): 653-672
Abstract
We use very deep U(n)GRI multifield imaging obtained at the Keck telescope to study the evolution of the rest-frame 1700 angstrom galaxy luminosity function as the universe doubles its age from z similar to 4 to similar to 2. We use exactly the same filters and color-color selection as those used by the Steidel team but probe significantl...More
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