Fig. 3.
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Our fit to the L- and N-band SED of T CrA. The L-band data are the average of the three MATISSE AT single-dish spectra taken in 2024, while the N-band spectrum was taken in 2008 by Spitzer. The SED of the central star is extracted from the SED modeling of Rigliaco et al. (2023). The dashed lines indicate the model SED interpolated between the L and N bands.
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