The HI-halo mass relation follows a double power-law with turnover near 10^11.2 solar masses; centrals dominate the HI budget below ~6e12 solar masses while satellites dominate above, and photometric members boost high-mass halo HI by 1.5-3x.
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DINGO/GAMA /WAVES: HI-halo mass relation
The HI-halo mass relation follows a double power-law with turnover near 10^11.2 solar masses; centrals dominate the HI budget below ~6e12 solar masses while satellites dominate above, and photometric members boost high-mass halo HI by 1.5-3x.