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Fig. 3.
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Same as in Fig. 2 but using 111 binary pulsars from the ATNF catalogue and assuming next-generation radio-telescope precision. We assume Tobs = 10 years, and a next-generation radio-telescope precision given by ϵ = 0.1 μs (based on the analysis presented in Liu et al. (2011) for the upcoming SKA)
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