Fig. C.1
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Spectral energy distribution of TOI-672, described in Section 3.1.4, assembled from broadband photometry obtained with APASS (magenta), SDSS (black), Gaia (green), 2MASS (yellow), WISE (red), and the Johnson system (blue). The horizontal bars indicate the effective wavelength ranges of each filter. The SED is fitted with a BT-Settl atmospheric model (Allard et al. 2012).
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