Fig. 7.
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Evolution with time of the global luminosity-weighted escape fraction of LyC photons fesc in SPHINX-CR (dark blue) and SPHINX-SN (red). The luminosity-weighted mean escape fraction fesc is shown in transparent lines, and the thick lines show the average over the last 100 Myr, to smooth the bursty fluctuations with time. In SPHINX-CR, the escape fraction of ionising radiation is lower than in SPHINX-SN.
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