Fig. B.1.
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Galaxy stamp cutout and SED for three representative galaxies in the sample. Left: 3x3 panels show the cutouts for the nine GLIMPSE JWST filters. Right: the observed photometry for that galaxy (black), the photometry obtained using Bayesian inference of CIGALE (red) and the best fit SED (grey). The three galaxies were selected for being bright, faint without strong magnification, and very-faint with strong magnification.
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