Open Access

Fig. 7.

image

G-band variability vs. GRP/GBP variability of all the sources selected in Sect. 2.1 (left) and of the sources selected in Sect. 4 (right). Eclipsing binaries have the same level variability in GBP and GRP and G−variability lower than 0.3. RR Lyrae stars have GBP/GRP variability ∼1.6 and G-band variability lower than 0.4.

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