Fig. 3.
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Comparison with HST data. Left: ForMoSA fits (dash lines) of HST G141 data (solid lines). We used the maximum (blue) and minimum (red) amplitude data from the sequence of Bowler et al. (2020). We also compared these HST data with our X-shooter data. Right: comparison between Teff posteriors from the HST’s fits (red and blue) and the fit of our X-shooter data (gray).
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