Traces of wobbling accretion disk in X-ray pulsar Her X-1 from observations of the ART-XC telescope of the SRG observatory

Open Access

Fig. 7.

χ² of the 4–12 keV pulse profile count rate deviations from constant constructed by the moving average method for time intervals of 4300 s with a 100 s shift. The green line corresponds to χ² = 1; the orange and red lines correspond to 2σ and 4σ flux deviations from constant, respectively.

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