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Fig. A.1.

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Calibrated MATISSE L- and LM-band data sets with pipeline produced uncertainties. First column: Correlated flux as a function of the spatial frequency. Second column: Closure phase as a function of the spatial frequency corresponding to the longest baselines of the triangles. Third column: Single-dish flux as a function of the wavelength. Fourth column: uv coverage of the observations. The correlated flux and the closure phase values are the average over the four non-chopped exposures of each observation, while the single-dish flux values are the average over the eight chopped exposures. The 2023 May 10 and 2024 June 2 data are UT observations, the rest are AT observations.

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