Fig. 5
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SED fit for the TOI-2458 system. The blue points with vertical error bars show the observed catalog fluxes and uncertainties from Gaia, TESS, Tycho-2, 2MASS, and WISE, while the horizontal error bars illustrate the width of the photometric band. For illustrative purposes, we overplot the best-matching Phoenix atmospheric model (Husser et al. 2013).
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