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Fig. 8.

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Fractional errors of the maximum likelihood HII bubble center (left) and radius (right) as a function of the number density of the observed galaxies. The black curve corresponds to a single realization of the EoR morphology and galaxy samples. The light (dark) blue region corresponds to the 95th (68th) percentile of fractional errors obtained from 100 realizations. With ngal≳0.01 galaxies cMpc−3, the fractional errors drop below the grid resolution we used to calculate the likelihoods (1.5 cMpc).

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