Fig. 8
EPIC-pn lightcurve of IGR J17451–3022 folded on the best orbital period determined in this work, 
s (see Sect. 4.1). The upper (middle) panel shows the folded source lightcurve in the soft (hard) X-ray energy band, while the bottom panel shows the HR (i.e., the ratio of the source count-rate in the hard, 2.5–12 keV, and soft, 0.5–2.5 keV, energy bands).
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