Fig. B.1.
Impact of the lower integration bound s0 for mean transmission curves. We averaged over all LOS and Lyα- emitting galaxy candidates at z = 3. We show the cases of f = 0.5, 1.0, 2.0, 2.5 around our fiducial case of 1.5. These results are contrasted with cases f = 10.0, 30.0 for interaction on large scales only. In addition, we show the case of a fixed s0 = 30 pkpc irrespective of virial radius of the underlying halo.
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