Fig. 5.
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Comparison of Lyman-α and UV circularized 90%-light radii. The figure shows the Lyman-α 90%-light radius. LLAMAS and UDF (Leclercq et al. 2017) galaxies are represented in red and grey, respectively. The UDF and LLAMAS values are both correlated (Spearman weighted p-value of p0 = 0.02 and p0 = 0.05 for UDF and LLAMAS, respectively). Both datasets are roughly centered around rLyα = 10 rUV.
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