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Fig. 5.

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UV slope plotted against EWLyα for the LAE+LBG sample. Orange dots represent UV slopes that, upon inspection, we find to be dubious: photometry that locally does not represent the slope well or has large errors. Red stars represent average values in equally sized bins between β = −3.5 and β = −1.0. The change in EWLyα across this range is not as significant as the change across the range of probed UV magnitudes (see Fig. 4); however, we see a lightly rising trend in EWLyα with bluer slopes down to β = −2.5.

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