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Fig. 1.


Stellar-to-halo mass relation for 110 galaxies in the SPARC sample. The points are colour-coded by the ratio of HI-to-stellar mass. The stellar-to-halo mass relation estimated by Moster et al. (2013) using abundance matching is shown as a black dashed curve; the scatter of the relation is shown shaded in grey. Galaxies that have converted all the available baryons in the halo into stars would lie on the long-dashed line, whose thickness encompasses uncertainties on fb. For reference, we also show the location of the Milky Way (cross) and of the Andromeda galaxy (plus) on the plot, as given by the modelling by Posti & Helmi (2019) and Corbelli et al. (2010), respectively.

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