Fig. 1.
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VST-SMASH sample properties. From top to bottom, the panels show the SFR, dynamical mass, H I gas mass, and Holmberg radius (in kiloparsecs) as functions of stellar mass for the VST–SMASH sample. The target analysed in this paper, IC 5332, is highlighted with black symbols. SFR- and MHI–M★ best-fit relations from Hunt et al. (2019) and Hunt et al. (2020) are also shown.
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