Fig. D.2.
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Spectral energy distribution of J0658. Valid fluxes from all available photometric surveys are shown. The best-fitting synthetic spectral model is overlaid as a gray line. Horizontal error bars represent the filter width at tenth maximum. (Data publications: Pan-STARRS1 (yellow): Chambers et al. 2016; 2MASS (salmon): Cutri et al. 2003; SkyMapper (green): Onken et al. 2019; and Gaia G/BP/RP (blue) and Gaia XP (light blue): Gaia Collaboration 2022).
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