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

Abstract

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 $0.8\pm 0.4$ $\mu s$ over the entire studied time interval. The fractional instability of the difference ${}_{ens}$ $-$ TT(BIPM2011) over 15 years is ${\sigma }_z=(0.6\pm 1.6)\cdot 10^{-15}$, which corresponds to an upper limit for the energy density of the gravitational--wave background ${\Omega }_g{h}^2\sim 10^{-10}$ and variations in the gravitational potential $\sim 10^{-15}$ Hz at the frequency $2\cdot 10^{-9}$.

arXiv comment11 pages, 2 figures

References in corpus (8)

• TEMPO2, a new pulsar timing package. I: Overview
• The Parkes Pulsar Timing Array Project
• Limits on the Stochastic Gravitational Wave Background from the North American Nanohertz Observatory for Gravitational Waves
• Pulsar timing signal from ultralight scalar dark matter
• Development of a pulsar-based timescale
• Constraints on ultralight scalar dark matter from pulsar timing
• The optimal filters for the construction of the ensemble pulsar time
• Optimal Filtration and a Pulsar Time Scale

Cited by in corpus (1)

• Measuring clock jumps using pulsar timing