Fig. 1.
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Two intervals of the γ-ray light curve of PKS 1502+106 exhibiting the repeated pattern of flares for: a) Interval between 18 October 2018 and 17 November 2019, processed with a 3.35 d integration; b) Interval between 26 March 2011 and 30 November 2011, processed with a 2.11 d integration. Both curves are over-sampled in such a way that the time difference between two consecutive points equals half of the integration time. The dashed red line marks the arrival time of IC190730A.
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