MIGHTEE-H i: The MHi - M∗ relation of massive galaxies and the Hi mass function at 0.25 < z < 0.5

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Abstract

The relationship between the already formed stellar mass in a galaxy and the gas reservoir of neutral atomic hydrogen, is a key element in our understanding of how gas is turned into stars in galaxy haloes. In this paper, we measure the relation based on a stellar-mass selected sample at

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Pan, H., Jarvis, M. J., Heywood, I., Yasin, T., Maddox, N., Santos, M. G., … Rajohnson, S. H. A. (2025). MIGHTEE-H i: The MHi - M∗ relation of massive galaxies and the Hi mass function at 0.25 < z < 0.5. Monthly Notices of the Royal Astronomical Society, 544(2), 1710–1731. https://doi.org/10.1093/mnras/staf1857

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