Inclination-Independent Galaxy Classification
Jeremy Bailin, William E. Harris (McMaster University)

TL;DR
This paper introduces a new galaxy classification method that accounts for inclination effects, revealing an intermediate galaxy class and providing insights into galaxy evolution mechanisms.
Contribution
The method explicitly corrects for inclination effects, enabling clearer separation of galaxy types and unveiling the intermediate class, which was previously hidden.
Findings
Inclination correction tightens parameter distributions.
Identifies a distinct intermediate galaxy class.
Suggests different evolutionary pathways for galaxy types.
Abstract
We present a new method to classify galaxies from large surveys like the Sloan Digital Sky Survey using inclination-corrected concentration, inclination-corrected location on the color-magnitude diagram, and apparent axis ratio. Explicitly accounting for inclination tightens the distribution of each of these parameters and enables simple boundaries to be drawn that delineate three different galaxy populations: Early-type galaxies, which are red, highly concentrated, and round; Late-type galaxies, which are blue, have low concentrations, and are disk dominated; and Intermediate-type galaxies, which are red, have intermediate concentrations, and have disks. We have validated our method by comparing to visual classifications of high-quality imaging data from the Millennium Galaxy Catalogue. The inclination correction is crucial to unveiling the previously unrecognized Intermediate class.…
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