Fig. 3.
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Bottom panels: light curves in WL folded on the orbital period of Eq. (1) (left) and on the pulse period of Eq. (6) (right). All individual relative WL fluxes are shown as green dots, and selected individual light curves are emphasized in black, red, and blue (see text). Top panels: mean light curves collected into 32 orbital bins (left) and pulse bins (right).
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