arXiv (All)
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Galaxy evolution in the post-merger regime. V - Atomic gas evolution traced by ALFALFA stacks
(Abridged) In this work, we investigate the role of atomic hydrogen (HI) gas in the galaxy merger lifecycle. In order to both identify galaxies in mergers, as well as to predict their time since coalescence, we present an extension of the MUlti Model Merger Identifier (MUMMI) machine vision pipeline
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