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Fig. 1.

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Radio timing observations obtained with the Lovell, Nançay, Parkes, and Westerbork telescopes. (a): timing observations as a function of observing frequency. (b) and (c): the residuals of the timing model as a function of orbital phase and time from observations with Lovell, Nançay, and Parkes. (d): the residuals of the timing model as a function of orbital phase from observations with Westerbork. The orbital phases covered by the WSRT observations is indicated with square brackets. Orbital phase ϕ = 0 is defined at the time of ascending node.

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