Fig. C.1.
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Results of testing the impact of an asymmetric scatter for the MHI − M⋆ relation. Top: MHI distributions (from which we have subtracted the median) in different stellar mass bins: 8.9 < log10(M⋆/M⊙) < 9.1 (solid green), 9.4 < log10(M⋆/M⊙) < 9.6 (dashed orange), 9.9 < log10(M⋆/M⊙) < 10.1 (dotted-dashed blue), and 10.4 < log10(M⋆/M⊙) < 10.5 (dotted purple). In dashed gray we show a lognormal random distribution obtained by assuming σ = 0.45, which is found to approximate all the MHI distributions well.
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