Fig. 7.
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Distribution of the sizes (in terms of HLR) of the Mg II halos. The halos were corrected by self-absorption before measuring their HLR using the absorption component of the best-fitting model. The radial profiles of the absorption-corrected Mg II emission halos are shown with a dashed line in Fig. 4. The HLR of each galaxy is provided in Table D.1.
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