JWST single-pixel spectral parameters obtained by our SED fitting using the Bagpipes package (Carnall et al. 2018, 2019) from pixel 13 to pixel 17 assuming the SED model from Table B.3. The figure depicts the star-formation rate (top panel), stellar mass (2nd panel, in units of 10¹⁰ M_⊙), mass-weighted age (third panel), and dust attenuation (bottom panel) per pixel. The uncertainties were computed from the posterior distributions at a 99.9% confidence level.