Fig. B.1.

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Recovered bubble maps corresponding to different galaxy number densities ngal≈0.0040−0.0005/cMpc3 at . To achieve these number densities we vary MUV, limit in our z = 8 simulations, and assume flux limit corresponding to a 5σ EW limit of 30 Å for the faintest galaxies. Dots show the detectable galaxies, color-coded by their true Lyα transmissions. As number density of galaxies increases, bubble recovery improves. With ngal≳0.002/cMpc3 we can recover bubbles well: lower ngal is not sufficient to sample the space.
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