The Baryonic Tully–Fisher Relation. I. WISE/Spitzer Photometry

The Baryonic Tully–Fisher Relation. I. WISE/Spitzer Photometry

We present Wide-field Infrared Survey Explorer (WISE) W1 photometry of the Spitzer Photometry and Accurate Rotation Curves sample. The baseline of near-IR fluxes is established for use by stellar mass models, a key component to the baryonic Tully–Fisher relation and other kinematic galaxies scaling...

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Bibliographic Details
Main Authors: Francis Duey, James Schombert, Stacy McGaugh, Federico Lelli
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astronomical Journal
Subjects:
Galaxy structure
Galaxy photometry
Disk galaxies
Online Access:https://doi.org/10.3847/1538-3881/ad454c

Internet

https://doi.org/10.3847/1538-3881/ad454c

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