The SAMI galaxy survey: predicting kinematic morphology with logistic regression

ABSTRACT We use the SAMI (Sydney-AAO Multi-object Integral field spectrograph) galaxy survey to study the the kinematic morphology–density relation: the observation that the fraction of slow rotator galaxies increases towards dense environments. We build a logistic regression model to quantitatively...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2024-02, Vol.528 (4), p.5852-5863
Hauptverfasser: Vaughan, Sam P, van de Sande, Jesse, Fraser-McKelvie, A, Croom, Scott, McDermid, Richard, Liquet-Weiland, Benoit, Barsanti, Stefania, Cortese, Luca, Brough, Sarah, Sweet, Sarah, Bryant, Julia J, Goodwin, Michael, Lawrence, Jon
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Sprache:eng
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