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Fig. C.2.
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Spectral energy distribution of J1903-0023. The best-fit model is plotted in grey. Photometric values are taken from 2MASS (Cutri et al. 2003), IGAPS (Monguió et al. 2020), Pan-STARRS (Chambers et al. 2016), Skymapper DR4 (Onken et al. 2024), and UKIDSS DR6 (Lucas et al. 2008). The residuals are shown below.
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