The full near-infrared through millimeter spectral energy distribution of CEERS-DSFG-1 overplotted with several of the best-fit SEDs described in Section 3 along with the current photometric constraints. The detections used in the fits are represented by the solid circles, while 2σ upper limits are illustrated by the downward arrows (note that error bars are smaller than the symbols). We show the EAZY fit to near-IR data only at z = 5.5 in orange, CIGALE to near-IR data only at z = 13.5 in red, and the fiducial CIGALE joint fit at z = 5.1 in light green. While the three SEDs satisfactorily reproduce the JWST photometry (see zoom-in inset plot), only the joint fit at z = 5.1 reproduces the (sub)millimeter fluxes.