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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Bibliographic Details
Published in:arXiv.org 2022-12
Main Authors: 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
Format: Article
Language:English
Subjects:
Galaxies
Independent variables
Integral field spectroscopy
Outliers (statistics)
Radio astronomy
Radio observation
Red shift
Rotational spectra
Scattering
Spectrum analysis
Stellar mass
Stellar rotation
Tully-Fisher relation
Velocity
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Description
Summary: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
ISSN:2331-8422
DOI:10.48550/arxiv.2212.04728