Among UV-bright red-sequence galaxies at z about 0.06 to 0.4, the fraction classified as UV upturn increases with stellar mass and rises then falls with redshift, with the mass trend concentrated in retired/passive systems.
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UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?
Among UV-bright red-sequence galaxies at z about 0.06 to 0.4, the fraction classified as UV upturn increases with stellar mass and rises then falls with redshift, with the mass trend concentrated in retired/passive systems.