Lyman-break galaxies from GALEX (Burgarella+, 2007)

Details Lyman-break galaxies from GALEX (Burgarella+, 2007) Lyman-break galaxies from GALEX (Burgarella+, 2007)

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..83800986b&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/380/986. Originally published in: 2007MNRAS.380..986B

Physics

Galaxies: Uv-Excess, Ultraviolet, Redshifts

Scientific paper

Ultraviolet (UV) galaxies have been selected from the Galaxy Evolution Explorer deep imaging survey. The presence of a far-UV (FUV) drop-out in their spectral energy distributions (SEDs) proved to be a very complete (83.3 per cent) but not very efficient (21.4 per cent) tool for identifying Lyman break galaxies (LBGs) at z~1. In this paper, we explore the physical properties of these galaxies and how they contribute to the total star formation rate (SFR).
(2 data files).

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