Fig. 3
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MATISSE calibrated flux in the L, M, and N bands together with the ATLAS9 atmospheric model interpolated for each star by SPIPS at the specific pulsation phase of observations. The blue bars represent the photometry interpolated at the phase of the MATISSE observations by SPIPS. In the case of U Aql, the N-band flux is the correlated flux. See Sect. 4 for details of the calibration.
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