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Fig. 7.

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Results of the tests for the existence of a Lyα halo. Top panel: histogram of the flux S/Ns between r = rin and rCoG measured on the optimized Lyα NBs. Blue and gray histograms indicate galaxies above and below the threshold of S/N = 3 (black dashed line), Non-LAHs and LAH candidates, respectively. RID = 23135 has a negative S/N(rin − rCoG) and is counted as S/N(rin − rCoG) = 0 in the plot. Bottom panel: probability of the null hypothesis that the SB profile at r = rin − rCoG matches that of the target’s continuum-component profile vs. flux S/N between r = rin and rCoG for the LAH candidates. A black dashed line represents the border of LAHs and Non-LAHs.

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