Fig. 2.
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Mean SF vs. time lag τ for sources with more than five FoV transits in the G band in a preliminary version of the Gaia-CRF3 sample, including about 1 850 000 AGN candidates. The various colours correspond to different G ranges for which the mean SFs have been estimated. Dashed lines represent the best-fit models to the mean SFs according to Eq. (3).
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