Demonstration of the data from HST, JWST, Herschel, and ALMA, and the best-fit SED, for one of the galaxies in the sample. The wealth of photometric observations from the rest-frame UV to the FIR, in addition to the spectroscopic redshift, enables detailed SED fitting that can robustly constrain the PAH features. The filter transmission curves of the available photometric data for the sample are shown at the bottom. The SEDs of the full sample are available online at https://zenodo.org/records/13736532