Fig. 1.
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One-day averaged light curve obtained by the MAXI monitor (4–10 keV) during the IXPE observations of the source (dark blue points). The blue-shaded areas correspond to eclipse periods according to Falanga et al. (2015). The red shaded areas represent the IXPE observations with the corresponding count-rate light curves (2–8 keV) shown in zoomed-in panels.
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