Fig. 7

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Comparison of the spectral energy distributions of our retrieved models compared to the low-resolution GPI data from Chilcote et al. (2017) and GRAVITY data from GRAVITY Collaboration (2020). Since we do not retrieve radius, the flux of our models is scaled such that it matches the GPI flux in the K-band. The solid line shows the median value and the colored region shows the 16th and 84th percentiles.
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