Fig. 9
Results of the fit to the XMM–Newton (right side of the timeline) and NuSTAR (left side of the timeline) light curves of IGR J17329-2731 with a superposition of sinusoidal functions with harmonically related periods. The red curve represents the best fit model and the most accurately derived spin period of the source from the combined XMM–Newton + NuSTAR dataset is 6680 ± 3 s (1σ).
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