Fig. 8
Left panel: mean absolute deviation of the flare phases as a function of orbital period. Right panel: mean absolute deviation of the flare phases multiplied by the orbital period as a function of orbital period. The dataset is that of orbital detections (o, filled black triangles). The empty triangles are obtained by simulating a population of flares for IGR J16479−4514 and IGR J16418−4532 unaffected by the presence of the eclipse.
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