Fig. 2.
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Post-fit residuals of ToAs from Arecibo data (with Mock and PUPPI backends) and FAST data (with ROACH backend) as a function of year (below) and orbital phase of pulsar (top). Different colours show residuals for different backends. Points labelled Mock-1 and Mock-2 show different sets of timing observations with the Mock spectrometers (see Table 1).
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