Fig. 1.
Source and background light curves of the eclipse observation #74 using 100 s bins. Top panel: source+background (black) and background (red) light curves extracted in the 0.5–12 keV energy range using circular regions with equal area. Bottom panel: full CCD light curve in the 10–12 keV energy range excluding the source region. The black vertical lines indicate split times for eclipse (a), egress (b), and out-of-eclipse (c) periods, according to (Coley et al. 2015) ephemeris. The full (dashed) horizontal line corresponds to the background rate of 1 cps (0.4 cps).
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