Fig. 21.

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How the measured isophotal Lyα halo scale length () varies with the stellar mass, total Lyα luminosity (LLyα), total FUV luminosity (LFUV), the size of the star forming regions (rSFRD > 0.01), and the centroid shift (ΔC). The measured Spearman’s coefficient and p-value between
and each quantity are displayed in the corresponding panels.
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