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Fig. 6

image

Left panel: Lyα escape fraction as a function of redshift for the bright (gray diamonds) and faint (gray triangles) volume limited samples. Strong Lyα emitters with EW0> 25 Å and EW0> 55 Å are shown with cyan and magenta empty circles, respectively. Objects with formally negative equivalent width of Lyα, corresponding to negative Lyα luminosity, are set here to log [ fesc(Lyα) ] = − 3. The big red and blue circles indicate the median escape fraction for the galaxies with EW0 [ Lyα ] > 55 Å and EW0 [ Lyα ] > 25 Å, respectively. The black (gray) arrows indicate the fesc(Lyα) below which 80% of the bright (faint) objects lie. Right panel: Lyα escape fraction as a function of the E(BV). The symbols are the same than in the left panel. The green dashed line shows the prediction by Verhamme et al. (2006).

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