Same as Fig. 2, but for the middle 6 sources in order of RID. Each row shows a different object. Panels a–f: are the same as those of Fig. 2. We note that the emission rings shown in the NB of RID = 9944 is caused by the mask for a source with extended emission. Although the ring feature of RID = 9944 overlaps with r = r_in − r_CoG, this object is not included in the isolated sample (as well as RID = 7876), and the main conclusion about the Lyα halo fraction is not affected by the ring.