CATALOG OF ULTRA-DIFFUSE GALAXIES IN THE COMA CLUSTERS FROM SUBARU IMAGING DATA

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Illuminating Low Surface Brightness Galaxies with the Hyper Suprime-Cam Survey (2017, methodology): “For comparison, the black line shows the same distribution for a sample of 753 UDGs in the Coma cluster (Yagi et al. 2016).”
(Almost) Dark Galaxies in the ALFALFA Survey: Isolated H i-bearing Ultra-diffuse Galaxies (2017, background): “Like other UDGs, they may be star-poor, failed ∼L? galaxies with suppressed star formation laws, or they may be H i-rich, extended dwarfs that only recently acquired their gas.”
NIHAO - XI. Formation of ultra-diffuse galaxies by outflows (2016, methodology): “…1000 UDGs have been identified in the Coma cluster using the Dragonfly array (van Dokkum et al. 2015a,b) and the Subaru telescope (Koda et al. 2015; Yagi et al. 2016): they represent a passively evolving population, lying on the red sequence in the color-magnitude diagram, as opposed to classical…”
Constraining the galaxy–halo connection over the last 13.3 Gyr: star formation histories, galaxy mergers and structural properties (2017, background): “Note, however, that most of the UDGs have been discovered in massive clusters (particularly in the Coma Cluster van Dokkum et al. 2015a; Yagi et al. 2016), with very few examples in the field (e.g., Mart́ınezDelgado et al. 2016).”