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Fig. 7


Analysis (i): lowest value of reduced χ2 () for each value of ReqRp (left panel) and stellar mass (middle panel) from the HDUST fit to the VEGA V2 data (642.5 nm band). Local regression fits to , as a function of the parameter values, are shown in red line. In the right panel, the predicted visibility from our best-fit HDUST model (red points; Table 5) is compared to the VEGA V2 measurements in the continuum band (black points). The predicted visibility from the HDUST model with the highest mass in the BeAtlas grid (14.6 M, highest in the middle panel) is shown in blue points.

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