Fig. A.1
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Gaia DR3 measurements of vsini_esphs versus each of the five covariates as indicated for the 384 γ Dor (grey triangles) and 1104 SPB (cyan squares) stars for which these quantities are available. The lower right panel shows the standard deviation of vbroad as a function of vsini_esphs for the 100 γ Dor and 190 SPB stars for which these quantities are available. When invisible, the errors are smaller than the symbol sizes.
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