WALLABY Pilot Survey: kNN identification of perturbed galaxies through H 1 morphometrics
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DOI: 10.1017/pasa.2025.5
Abstract: Abstract Galaxy morphology in stellar light can be described by a series of ‘non-parametric’ or ‘morphometric’ parameters, such as concentration-asymmetry-smoothness, Gini, $M_{20}$ , and Sérsic fit. These parameters can be applied to column density maps… read more here.
Keywords: pilot survey; morphometrics; wallaby pilot; perturbed galaxies ... See more keywords