Dust-, ISM-, and IGM-corrected model spectra of the candidates, as well as observed (filled circles) and model predicted (open circles). Orange spectra are the BAGPIPES best fit to the observed data points. Model spectra generated from the same best-fit parameters, but with ISM and dust removed, are shown in black. Gray spectra show the ISM- and dust-free model spectra corrected for the BAGPIPES assigned average redshift-dependent IGM absorption.