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Fig. 13.

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Distribution of fLyα, full FOVfLyα, tile fit for our HzRGs. The fLyα, full FOV is the intrinsic Lyα flux resulted from fitting the spectrum summed over the entire FOV. The ΣfLyα, tile fit is the summation of the intrinsic Lyα flux in each tessellation bin (Fig. 1b). The smaller the value, the more likely the Lyα photon is being double-counted when correcting for absorption. 4C+04.11 is the one with the smallest ratio which may also indicate over-correction (Appendix B).

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