High-energy characteristics of the accretion-powered millisecond pulsar IGR J17591−2342 during its 2018 outburst - XMM-Newton, NICER, NuSTAR, and INTEGRAL view of the 0.3–300 keV X-ray band

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Fig. 9.

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IGR J17591−2342 late-time INTEGRAL-ISGRI (20–60 keV) outburst profile starting from MJD 58379 with a time bin size of 0.5 d. The dashed line corresponds to the best fit in terms of an exponential profile, F ∝ e^{−t/9^d}, until the break (“knee”) followed by a linear decay.

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