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The Luminosity Function for L>L* Galaxies at z > 3

Matthew A. Bershady·Steven R. Majewski·David C. Koo·Richard G. Kron·Jeffrey A. Munn
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Abstract

Through use of multiband (U, B, R, I) photometry we have isolated high redshift (3.0 L* luminosity function for z = 3-5 galaxies obtained by a photometric redshift analysis of the Hubble Deep Field (HDF) by Gwyn & Hartwick (1996). Our results at R ~ 23 are more consistent with the photometric redshift analysis of the faint HDF galaxies by Sawicki & Yee (1996), but our present upper limits at the brightest magnitudes (R < 21.5, M(R) < -24) allow more generous volume densities of these super-L* galaxies.

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Matthew A. Bershady, Steven R. Majewski, David C. Koo, Richard G. Kron, Jeffrey A. Munn. 1997-09-22. The Luminosity Function for L>L* Galaxies at z > 3. https://doi.org/10.1086/310995

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