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Fig. 9


Relation between log (SFRSED) and log (SFRLyα/SFRSED) for galaxies with detected Lyα emission, assuming a declining (red dots) and a constant SFH (blue dots). Lyα luminosities have not been corrected for dust. The dashed line shows log (SFRLyα) = log (SFRSED). We recall that SFRLyα is a lower limit to the true SFR (see text).

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