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

By Kaila Ronayne and others at
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Logo42 US
We test the relationship between UV-derived star formation rates (SFRs) and the 7.7 {\mu}m polycyclic aromatic hydrocarbon (PAH) luminosities from the integrated emission of galaxies at z ~ 0 - 2. We utilize multi-band photometry covering 0.2 - 160 {\mu}m from HST, CFHT, JWST, Spitzer, and Herschel for galaxies in... Show more
October 13, 2023
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CEERS: 7.7 $μ$m PAH Star Formation Rate Calibration with JWST MIRI
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