Gas-rich galaxies follow a single Schechter stellar mass function; abundance matching the HI and stellar mass functions yields a selection-corrected M_HI-M_star relation.
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The Stellar Mass Function of Gas-Rich Galaxies and the Underlying $M_{\rm HI}-M_{\rm star}$ Scaling Relation in the Local Universe
Gas-rich galaxies follow a single Schechter stellar mass function; abundance matching the HI and stellar mass functions yields a selection-corrected M_HI-M_star relation.