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The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.6 and 1.2

By M. Page and others
We use ultraviolet imaging taken with the XMM-Newton Optical Monitor telescope (XMM-OM), covering 280 square arcminutes in the UVW1 band (effective wavelength 2910 Angstroms) to measure rest-frame ultraviolet (1500 Angstrom) luminosity functions of galaxies with redshifts z between 0.6 and 1.2. The XMM-OM data are supplemented by a large body... Show more
June 15, 2021
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The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.6 and 1.2
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