For pulsars orbiting stellar or intermediate-mass black holes, standard post-Newtonian timing formulas can differ from a full general-relativistic computation by 10^-7 to 10^-4 seconds, enough to affect future SKA timing.
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Towards an exact approach to pulsar timing
For pulsars orbiting stellar or intermediate-mass black holes, standard post-Newtonian timing formulas can differ from a full general-relativistic computation by 10^-7 to 10^-4 seconds, enough to affect future SKA timing.