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Fig. 4.

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Variation in spectral parameters with phase for Obs. 1, including the central energy (E1/E2), width (σ1/σ2), and depth (Depth1/Depth2) of the cyclotron absorption line (and its harmonics), the central energy (EFe), line width (σ), and normalization (Ngau) of the iron line, and the plasma temperature (kT), plasma optical depth (τ), and normalization (Ncomp) of the compTT component. The gray line represents the average profile of the data used for the phase-resolved spectral analysis. The triangles indicate the upper limits.

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