CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI

CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI

We test the relationship between UV-derived star formation rates (SFRs) and the 7.7 μ m polycyclic aromatic hydrocarbon luminosities from the integrated emission of galaxies at z ∼ 0–2. We utilize multiband photometry covering 0.2–160 μ m from the Hubble Space Telescope, CFHT, JWST, Spitzer, and Her...

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Bibliographic Details
Main Authors: Kaila Ronayne, Casey Papovich, Guang Yang, Lu Shen, Mark Dickinson, Robert Kennicutt, Anahita Alavi, Pablo Arrabal Haro, Micaela B. Bagley, Denis Burgarella, Aurélien Le Bail, Eric F. Bell, Nikko J. Cleri, Justin Cole, Luca Costantin, Alexander de la Vega, Emanuele Daddi, David Elbaz, Steven L. Finkelstein, Norman A. Grogin, Benne W. Holwerda, Jeyhan S. Kartaltepe, Allison Kirkpatrick, Anton M. Koekemoer, Ray A. Lucas, Benjamin Magnelli, Bahram Mobasher, Pablo G. Pérez-González, Laura Prichard, Marc Rafelski, Giulia Rodighiero, Ben Sunnquist, Harry I. Teplitz, Xin Wang, Rogier A. Windhorst, L. Y. Aaron Yung
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Star formation
Polycyclic aromatic hydrocarbons
James Webb Space Telescope
Hubble Space Telescope
Galaxy evolution
Infrared galaxies
Online Access:https://doi.org/10.3847/1538-4357/ad5006

Internet

https://doi.org/10.3847/1538-4357/ad5006

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