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