Fig. 1
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Top: right ascension and declination map distribution of the Gaia targets possessing a Gaia rotation period from DR2 or DR3 and an EVEREST K2 light curve. The magnitude G is colour-coded. The full sample of Gaia targets with a rotation period in DR3 is shown for reference (Distefano et al. 2023) with their density colour-coded in orange. The location of the Kepler field is shown in grey. Bottom: same for the galactic location of the targets.
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