The Ultraviolet Galaxy Luminosity Function in the Local Universe from GALEX Data

  • Wyder T
  • Treyer M
  • Milliard B
  • et al.
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Abstract

We present the results of a determination of the galaxy luminosity function at ultraviolet wavelengths at redshifts of z = 0.0-0.1 from Galaxy Evolution Explorer (GALEX) data. We determined the luminosity function in the GALEX far-UV and near-UV bands from a sample of galaxies with UV magnitudes between 17 and 20 that are drawn from a total of 56.73 deg2 of GALEX fields overlapping the bJ-selected Two-Degree Field Galaxy Redshift Survey. The resulting luminosity functions are fainter than previous UV estimates and result in total UV luminosity densities of 10 25.55±0.12 and 1025.72±0.12 ergs s -1 Hz-1 Mpc-3 at 1530 and 2310 Å, respectively. This corresponds to a local star formation rate density in agreement with previous estimates made with Hα-selected data for reasonable assumptions about the UV extinction.

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Wyder, T. K., Treyer, M. A., Milliard, B., Schiminovich, D., Arnouts, S., Budavári, T., … Welsh, B. Y. (2005). The Ultraviolet Galaxy Luminosity Function in the Local Universe from GALEX Data. The Astrophysical Journal, 619(1), L15–L18. https://doi.org/10.1086/424735

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