Fig. 6
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Observed photometry of KOI-3886 (empty black circles), and a 1T-model fit of a Kurucz model (Kurucz 1979) with Teff = 4750 K and logg* = 2.5 (red crosses and solid pale red line). Whereas the red part of the SED is well reproduced by the model, the fluxes below ~ 5000 Å, and in particular that corresponding to the NUV GALEX band, are underestimated.
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