Characterization of Two Cool Galaxy Outflow Candidates Using Mid-infrared Emission from Polycyclic Aromatic Hydrocarbons

Journal:

The Astrophysical Journal Letters

Published:

2025-10-03

DOI:

10.3847/2041-8213/ae08b7

Affiliations:

26

Authors:

25

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Institutions	Authors	Share
The Ohio State University (OSU), United States of America (USA)	3.000000	0.12
University of California, San Diego (UC San Diego), United States of America (USA)	2.000000	0.08
University of Wyoming, United States of America (USA)	2.000000	0.08
Johns Hopkins University (JHU), United States of America (USA)	2.000000	0.08
Heidelberg University (Uni Heidelberg), Germany	1.666667	0.07
Whitman College (Whitman), United States of America (USA)	1.000000	0.04
Ghent University (UGent), Belgium	1.000000	0.04
Joint Space-Science Institute (JSI), United States of America (USA)	1.000000	0.04
University of Oxford, United Kingdom (UK)	1.000000	0.04
University of Arkansas (UARK), United States of America (USA)	1.000000	0.04
J-L Lagrange Laboratory, France	1.000000	0.04
Max Planck Institute for Extraterrestrial Physics (MPE), Germany	1.000000	0.04
University of Cape Town (UCT), South Africa	1.000000	0.04
Tamkang University (TKU), Taiwan	1.000000	0.04
NSF's NOIRLab, United States of America (USA)	1.000000	0.04
University of Alberta (U of A), Canada	1.000000	0.04
Max Planck Institute for Astronomy (MPIA), Germany	1.000000	0.04
Space Telescope Science Institute (STScI), United States of America (USA)	1.000000	0.04
European Southern Observatory (ESO), Germany	0.500000	0.02
Lyon Centre for Astrophysics Research (CRAL), France	0.500000	0.02
Harvard-Smithsonian Center for Astrophysics (CfA), United States of America (USA)	0.333333	0.01

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