Fig. 4.

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Phase-folded light curves of AGL J1736−3250 and IGR J17354−3255. The zero phase ephemeris is MJD 52698.205 and the orbital period is (8.4474 ± 0.0017) d. Phase 0 is at periastron passage. From top to bottom: (a) Histogram of the number of flares detected by AGILE as reported in Table 2; (b) AGILE/GRID 0.1 − 10 GeV phase-folded light curve (1σ errors and upper limits), that results variable at 99% confidence level (see text); (c) INTEGRAL/IBIS 18 − 60 keV phase-folded light curve of IGR J17354−3255 (Sguera et al. 2011; d) Swift/BAT 14 − 195 keV phase-folded light curve of IGR J17354−3255; (e) Swift/XRT 0.3 − 10 keV phase-folded light curve of IGR J17354−3255 (Ducci et al. 2013).
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