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Fig. 14.
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Photometric amplitude A1 in the Gaia G-band as a function of the v sin i derived from spectroscopic Gaia DR3 data for a sample of 3515 δ Sct stars. The dark blue line is the median amplitude for each v sin i bin of 15 km s−1 while the light blue band shows the 25%–75% quantile interval.
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