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Using data from the Parkes radio telescope, we observe a smooth and fast spin-down process subsequent to the X-ray bursts resulting in a net change in the pulsar rotational frequency of $\\Delta\\nu\\approx-4\\times10^{-4}$\\,Hz. During the transition, a net spin-down rate increase of $\\Delta\\dot\\nu\\approx-1\\times10^{-10}$\\,Hz\\,s$^{-1}$ is observed, followed by a return of $\\dot{\\nu}$ to its original value. 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