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PAH emission from star-forming and quiescent galaxies at $z=0.5-0.8$ probed by JWST/MIRI

Mondal, Chayan et al.
arXiv (All) · Papers
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astrophysics-of-galaxies
We investigate emission from polycyclic aromatic hydrocarbon (PAH) dust molecules in 224 MIRI-selected star-forming and quiescent galaxies at $z=0.5-0.8$ in the GOODS-South field using multi-wavelength data from the AstroSat/UVIT, JWST, HST, Herschel, and MUSE. We define an observed diagnostic param
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