The Calibration of Short-wavelength Polycyclic Aromatic Hydrocarbon Emission as Star Formation Rate Indicators with JWST

We use JWST/NIRCam and MIRI imaging acquired by the Feedback in Emerging extrAgalactic Star clusTers (or FEAST) program along with archival Hubble Space Telescope imaging to map ionized gas (Pa α , Br α , and H α ) and polycyclic aromatic hydrocarbon (PAH) emission (3.3 and 7.7 μ m) across a sample...

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Bibliografiset tiedot

Päätekijät:	Benjamin Gregg, Daniela Calzetti, Angela Adamo, Alex Pedrini, Sean T. Linden, Varun Bajaj, Jenna E. Ryon, Arjan Bik, Giacomo Bortolini, Matteo Correnti, Bruce T. Draine, Bruce G. Elmegreen, Helena Faustino Vieira, John S. Gallagher, Kathryn Grasha, Kelsey E. Johnson, Thomas S.-Y. Lai, Matteo Messa, Göran Östlin, Linda J. Smith, Monica Tosi
Aineistotyyppi:	Artigo
Kieli:	Inglês
Julkaistu:	IOP Publishing 2026-01-01
Sarja:	The Astrophysical Journal
Aiheet:	Galaxies H II regions Interstellar dust Interstellar medium James Webb Space Telescope Polycyclic aromatic hydrocarbons
Linkit:	https://doi.org/10.3847/1538-4357/ae1ca8
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