Fig. 1.
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NuSTAR 3–79 keV flux for observation I (blue) in January 2019 and observation II in May 2019 (red) with a time resolution of PI = 283.4532 s and PII = 283.4447 s, respectively, and Swift/BAT 15–50 keV flux averaged over all data since 2005 (solid black line) plotted over the neutron star’s orbital phase, where ϕorb = 0 is defined with T90.
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