Discovery of a 0.8-mHz quasi-periodic oscillation in the transient X-ray pulsar SXP31.0 and associated timing transitions

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Fig. 6.

Dependence of the PF on energy. The dashed red line marks the energy above which secondary peaks disappear from the pulse profile in NuObs1, coinciding with the onset of a growth in the PF (see Sect. 3.1.2). L₃₈ is the bolometric luminosity in units of 10³⁸ erg s⁻¹.

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