The limitations (and potential) of non-parametric morphology statistics for post-merger identification

ABSTRACT Non-parametric morphology statistics have been used for decades to classify galaxies into morphological types and identify mergers in an automated way. In this work, we assess how reliably we can identify galaxy post-mergers with non-parametric morphology statistics. Low-redshift (z ≲ 0.2),...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2024-02, Vol.528 (4), p.5558-5585
Hauptverfasser:	Wilkinson, Scott, Ellison, Sara L, Bottrell, Connor, Bickley, Robert W, Byrne-Mamahit, Shoshannah, Ferreira, Leonardo, Patton, David R
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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