The sloan digital sky survey u-band galaxy survey: luminosity functions and evolution

Abstract

We construct and analyse a u-band selected galaxy sample from the Sloan Digital Sky Survey (SDSS) Southern Survey, which covers 275 deg(2). The sample includes 43 223 galaxies with spectroscopic redshifts in the range 0.005 < z < 0.3 and with 14.5 < u < 20.5. The signal-to-noise (S/N) ratio in the u-band Petrosian aperture is improved by co-adding multiple epochs of imaging data and by including sky-subtraction corrections. Luminosity functions for the near-UV(0.1)u band (lambda approximate to 322 +/- 26 nm) are determined in redshift slices of width 0.02, which show a highly significant evolution in M* of -0.8 +/- 0.1 mag between z = 0 and 0.3; with M 5 log h(70) = 18.84 +/- 0.05 (ABmag), log = 2.06 +/- 0.03 (h(70)(3) Mpc(-3)) and log p(L) = 19.11 +/- 0.02 (h(70) W Hz(-1) Mpc(-3))at z = 0.1. The faint-end slope determined for z < 0.06 is given by alpha = 1.05 +/- 0.08. This is in agreement with recent determinations from the Galaxy Evolution Explorer at shorter wavelengths. Comparing our z < 0.3 luminosity density measurements with 0.2 < z < 1.2 from Classifying Objects by Medium Band Observations in 17 Filters (COMBO-17), we find that the 280-nm density evolves as p(L) alpha (1 + z)(beta) with beta = 2.1 +/- 0.2; and find no evidence for any change in slope over this redshift range. By comparing with other measurements of cosmic star formation history, we estimate that the effective dust attenuation at 280 nm has increased by 0.8 +/- 0.3 mag between z = 0 and 1.d 1.