Fig. 22.
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Comparison between MATISSE N band and MIDI data obtained on the classical Be star α Arae using the UTs. Left: all data plotted as a function of the spatial frequency with a best unresolved + uniform disk model. Centre: corresponding uv plane coverage with the same colours for MIDI and MATISSE observations. Right: data plotted as a function of the wavelength for two similar baselines in terms of length and orientation.
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