The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.6 and 1.2
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DOI: 10.1093/mnras/stab1638
Abstract: We use ultraviolet (UV) imaging taken with the XMM–Newton Optical Monitor telescope (XMM-OM), covering 280 arcmin2 in the UVW1 band (λeff = 2910 Å) to measure rest-frame UV 1500-Å luminosity functions of galaxies with redshifts z between 0.6… read more here.
Keywords: luminosity; galaxies redshifts; luminosity function; star forming ... See more keywords