Fig. 4.
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Upper panel: Ωneutral evolution for the non-equilibrium H2-based star formation model (red dashed line, HM-HISSmed-H2) with an HM background and compared to the reference run (solid black line, HM-HISSmed). Lower panel: corresponding ΩH2 evolution. Observational determinations are listed in Table A.1 (see also text and Fig. 3).
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