Fig. 6.

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Comparison of the derived SFRs for our LAE+LBG sample, colour-coded by redshift. The errors on the SFRLyα are smaller than the size of the points in most cases. The dashed blue line denotes a one-to-one SFR ratio, i.e., SFRUV = SFRLyα. Galaxies along this line also have equal escape fractions: fesc, UV = fesc, Lyα. Most of our sample lies under this line, and the dashed red line denotes the median SFR ratio of our sample, 0.35. For fainter objects with SFRUV < 1 M⊙ yr−1, a greater fraction lie above the line of equal SFR, a trend previously observed in Ando et al. (2006), Schaerer et al. (2011), and dLV20.
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