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Fig. B.1
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S/N and TOA uncertainty ratios as a function of time for PSRs J0125 - 2327, J0613-0200, J1022+1001, and J1024-0719. The S/N and TOA uncertainty values were derived from 1.4 GHz NUPPI observations calibrated using the IFA method and the calibration method presented in Sect. 3 (see Sect. 4.1 for details on the analysis).
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