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Ultraviolet and Far‐Infrared–selected Star‐forming Galaxies atz = 0: Differences and Overlaps
2006
Astrophysical Journal
We study two samples of local galaxies, one is UV (GALEX) selected and the other FIR (IRAS) selected, to address the question whether UV and FIR surveys see the two sides ('bright' and 'dark') of the star formation of the same population of galaxies or two different populations of star forming galaxies. No significant difference between the L_tot (=L_60+L_FUV) luminosity functions of the UV and FIR samples is found. Also, after the correction for the 'Malmquist bias' (bias for flux limited
doi:10.1086/504974
fatcat:isjgnhda4fd4zasocuehjqccmu