Fig. 7.
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Fraction of (secure) outflow candidates as a function of stellar mass. The fraction is determined per stellar mass bin with widths of Δlog10(M⋆/M⊙) = 0.5 that contain a minimum of 3 galaxies. Each level represents the fraction of outflow candidates relative to all galaxies in the mass bin. The total amount of galaxies per mass bin is given at the bottom of each bin.
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