Evolution of the spectral parameters of individual pulses. a) Light curve between 0.5 − 10 keV; b) Fe Kα flux (including the Compton shoulder); c) Fe Kβ flux; d) Ni Kα flux; e) ratio between the Compton shoulder and the Gaussian shaped Fe Kα line; and f) ratio between the Fe Kα and the Fe Kβ flux. The fluxes of the lines are given in photons s-1 cm-2 × 10-3.
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