Fig. 1.
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Pulse TOAs obtained from the RXTE/PCA observations after the removal of the overall spin-up trend (see text), shown at the top. Pulse profile evolution of MXB 0656–072, sorted by 3–20 keV RXTE/PCA luminosity (bottom). To improve legibility, the pulse profiles have been normalised to [0, 1] range and displayed for two complete cycles.
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