Fig. 2
Distribution of the Gaia DR2 RR Lyrae candidates confirmed by the Kepler (targeted and FFI) and K2 measurements in the sky, mapped in a Mollweide projection of equatorial coordinates. The thick line in light blue marks the Galactic equator, and the colour-coding shows the number of Gaia FoV transits in the G band per star. The original Kepler field is the northernmost group of stars at RA ≈ 300 deg.
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