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Fig. B.1.


Figure outputs of the atlas. Data taken with the UTs and ATs are marked with circles and diamonds, respectively. Top: uv-coverage plot. Data shown with small symbols are flagged as unreliable. Middle: Gaussian size diagram. The plot shows the physical sizes of the disk (HWHM, in au, see Eq. (2)) individually measured for each observation corresponding to different baseline angles. Bottom: results of the interferometric modeling to the correlated and total fluxes (shown at 0 m baseline) at 10.7 μm as a function of baseline length. Blue solid line: continuous model fit. Blue dashed line: gapped model fit. Red and green lines show the correlated fluxes extrapolated from the continuous model to the K and L bands, respectively. Dotted lines show the estimates for the unresolved stellar emission. Data points on each subplot are color-coded for observation date.

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