Attenuation maps (A_λ; left side) and their respective uncertainties (ΔA_λ; right side). Top row: attenuation calculated from the HST F606W filter, whose reference wavelength is 0.606 μm. Middle row: attenuation calculated from the JWST F090W filter, whose reference wavelength is 0.90 μm. Bottom row: attenuation calculated from the JWST F150W filter, whose reference wavelength is 1.50 μm. All maps are overlaid (green for A_λ and white for ΔA_λ) with their respective S/N maps (that is, the HST F606W and JWST F090W and F150W filters each have their own S/N maps, not given in this paper) as a contour such that S/N_λ ≥ 1. All contour maps are smoothed over (3 pixels across). Also overlaid in black is the Petrosian radius (R_P =  12 kpc). These attenuation structures are well outside the stellar disk.