Fig. C.1.
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Intrinsic (top) and escaping (bottom) ionising emissivities as a function of halo mass Mh for the evolving IMF (left) and Salpeter IMF (right) models at z = 6 (dark blue), 8 (violet), and 12 (orange). Solid lines show the median ionising emissivity and transparent shaded coloured regions the 1 − σ limits of the ionising emissivity values at a given halo mass.
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