Fig. 11.
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Instantaneous star formation efficiency as a function of halo mass for the three redshift bins in our sample. Solid lines and shaded regions show the estimates from Shuntov et al. (2025a), based on the UV luminosity function and halo occupation distribution (HOD) modeling. Our estimates of ϵ do not show any strong variation with redshift and confirm the low values obtained by Shuntov et al. (2025a).
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