Best-fit rest-frame SED of J044232.92. The red points represent the observed photometric data points, and the one with a downwards pointing arrow marks the λ_obs = 22 μm upper flux density limit, which is taken into account in the fit. The blue line is the best-fit MAGPHYS+photo-z model SED (Battisti et al. 2019). For comparison, the far-IR to submillimetre SED of G169.20-8.96 is shown with green points indicating the IRAS 100 μm and Planck photometric data points and the green dashed line representing a single-temperature modified blackbody fit to those data (see text for details).