Summary of prospector SED model. Panel a: Triangle diagram with the marginalized posterior distribution over a subset of the model-free or dependent parameters (see Table 2 for a description of the parameters and their probability prior). Panel b: SED, including wide- and medium-band measured flux densities (diamonds), the spectrum (grey line with grey region as the uncertainty). NIRCam, MIRI and ALMA data are in black, blue and pink, respectively. Model predictions are red circles (flux densities) or the red line (spectrum). The sand-coloured line is the model SED without convolving to the spectral resolution fo the data. Panel c: Model residuals normalised by the uncertainties. Panel d: Same as panel b, but for the FIR region. The orange square is the ALMA [O III]flux. Panel e: Same as panel c, but for the FIR region. Panel f: Star-formation history (red), with the prior probability in grey.