SAMI-HI: The HI view of the H$\alpha$ Tully-Fisher relation and data release

We present SAMI-HI, a survey of the atomic hydrogen content of 296 galaxies with integral field spectroscopy available from the SAMI Galaxy Survey. The sample spans nearly 4 dex in stellar mass ($M_\star = 10^{7.4}-10^{11.1}~ \rm M_\odot$), redshift $z

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Hauptverfasser: Catinella, Barbara, Cortese, Luca, Tiley, Alfred L, Janowiecki, Steven, Watts, Adam B, Bryant, Julia J, Croom, Scott M, d'Eugenio, Francesco, van de Sande, Jesse, Bland-Hawthorn, Joss, Fraser-McKelvie, Amelia, Richards, Samuel N, Sweet, Sarah M, Pisano, Daniel J, Pingel, Nickolas, Koopmann, Rebecca A, Cottrill, Dillion, Hill, Meghan
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Sprache:eng
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Zusammenfassung:We present SAMI-HI, a survey of the atomic hydrogen content of 296 galaxies with integral field spectroscopy available from the SAMI Galaxy Survey. The sample spans nearly 4 dex in stellar mass ($M_\star = 10^{7.4}-10^{11.1}~ \rm M_\odot$), redshift $z
DOI:10.48550/arxiv.2212.04728