BAGPIPES SED fits for our two highest redshift candidates (the highest-z of which is confirmed by spectroscopy Weibel et al. 2025). The yellow points are the observed photometry and the grey points correspond to non-detections with S/N < 3. The red-squares correspond to the best-fit model photometry and the red line corresponds to the best-fit model spectrum. Uncertainties in the best-fit model spectrum are denoted by the shaded regions which correspond to the 16th and 84th percentiles of the resulting distribution. An RGB image of the galaxy corresponding to F115W-F200W-F444W is included in the upper right of the figure. Both galaxies have MIRI coverage constraining the NIR part of the SED.