A Pulsar Time Scale Based on Parkes Observations in 1995–2010

Resumo

Timing of highly stable millisecond pulsars provides the possibility of independently verifying terrestrial time scales on intervals longer than a year. An ensemble pulsar time scale is constructed based on pulsar timing data obtained on the 64-m Parkes telescope (Australia) in 1995–2010. Optimal Wiener filters were applied to enhance the accuracy of the ensemble time scale. The run of the time-scale difference PT_ens−TT(BIPM2011) does not exceed 0.8 ± 0.4 μs over the entire studied time interval. The fractional instability of the difference PT_ens−TT(BIPM2011) over 15 years is σ_z = (0.6 ± 1.6) × 10⁻¹⁵, which corresponds to an upper limit for the energy density of the gravitational-wave background Ω_gh² ~ 10⁻¹⁰ and variations in the gravitational potential ~10⁻¹⁵ Hz at the frequency 2 × 10⁻⁹ Hz.