Fig. A.1
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Amount of ionising photons for HI (QHI, left panel) and for He I (QHI, right panel) in the case of the β = 1 grid models (H19 & S19, black circles) and the PoWRHD models (red squares). Similar to Figs. 1, 2, and 5, a correction for GAIA DR3 parallaxes (grey circles) was made in order to separate the effects of distance updates and model differences, denoted by the grey arrows.
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