Fig. 6
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Relation between Teff and υ sin i from the log 𝑔-iterated SPC analysis. Here we have included only the stars with QF = 1, 2. Stars with filled blue markers have a Gaia EDR3 RUWE > 1.4. For stars with multiple observations, we have for the uncertainty on υ sin i added in quadrature the standardised MAD from individual observations relative to the S/N-weighted average.
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