Fig. 13
Distributions of normalised residuals (
of the squared visibility for our best-fit model with 
, while the total number of measurements is Nvis = 17 391. Four separate datasets are shown, corresponding to the MARKIII, NPOI, CHARA/VEGA, and VLTI/AMBER interferometers. The distributions are not perfectly symmetric about zero and for CHARA/VEGA data are significantly wider, probably due to unaccounted calibration uncertainties.
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