Systematically Measuring Ultra-diffuse Galaxies (SMUDGes). V. The Complete SMUDGes Catalog and the Nature of Ultradiffuse Galaxies
Affiliation
Steward Observatory, Department of Astronomy, University of ArizonaIssue Date
2023-07-25
Metadata
Show full item recordPublisher
American Astronomical SocietyCitation
Dennis Zaritsky et al 2023 ApJS 267 27Rights
© 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We present the completed catalog of ultradiffuse galaxy (UDG) candidates (7070 objects) from our search of the DR9 Legacy Survey images, including distance and total mass estimates for 1529 and 1436 galaxies, respectively, that we provide and describe in detail. From the sample with estimated distances, we obtain a sample of 585 UDGs (μ 0,g ≥ 24 mag arcsec−2 and r e ≥ 1.5 kpc) over 20,000 square degrees of sky in various environments. We conclude that UDGs in our sample are limited to 1010 ≲ M h /M ⊙ ≲ 1011.5 and are on average a factor of 1.5-7 deficient in stars relative to the general population of galaxies of the same total mass. That factor increases with increasing galaxy size and mass up to a factor of ∼10 when the total mass of the UDG increases beyond M h = 1011 M ⊙. We do not find evidence that this factor has a dependence on the UDGs large-scale environment. © 2023. The Author(s). Published by the American Astronomical Society.Note
Open access journalISSN
0067-0049Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.3847/1538-4365/acdd71
Scopus Count
Collections
Except where otherwise noted, this item's license is described as © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.