Fig. 1.
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Top panel: NICER 0.3–10 keV light curve of IGR J17511−3057 during the latest outburst starting from February 11, 2025 (MJD 60717.7). The count rate is estimated by collecting 50 s of exposure time. Middle panel: Temporal evolution of the fractional amplitude of the sinusoidal component used to model the source pulse profiles. Bottom panel: Pulse phase residuals in units of phase cycles relative to the best-fitting solution.
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