Pulse frequency variations and timing noise of MXB 0656–072 during the 2007–2008 type I outbursts and implications for its magnetic field

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Fig. 3.

Frequency measurements of MXB 0656–072 with RXTE/PCA (black) and Fermi/GBM (green) shown at the top. The solid red line represents the intrinsic spin frequency model obtained through the $\dot{ν}$ $\dot{\nu}$ –L relation. Middle panel: 3–20 keV RXTE/PCA flux evolution. Lower panel: spin frequency residuals after subtracting ν_model from the frequency measurements.

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