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Development of a pulsar-based time-scale

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posted on 2024-08-06, 10:21 authored by G. Hobbs, W. Coles, R. Manchester, M. J. Keith, Ryan ShannonRyan Shannon, D. Chen, Matthew BailesMatthew Bailes, N. D R Bhat, S. Burke-Spolaor, David J. Champion, A. Chaudhary, A. Hotan, J. Khoo, J. Kocz, Y. Levin, Stefan Oslowski, B. Preisig, V. Ravi, J. Reynolds, J. M. Sarkissian, Willem van Straten, J. P W Verbiest, D. Yardley, X. P. You
Using observations of pulsars from the Parkes Pulsar Timing Array (PPTA) project we develop the first pulsar-based time-scale that has a precision comparable to the uncertainties in International Atomic Time-scales (TAI). Our ensemble of pulsars provides an Ensemble Pulsar Scale (EPS) analogous to the free atomic time-scale Echelle Atomique Libre. The EPS can be used to detect fluctuations in atomic time-scales and therefore can lead to a new realization of Terrestrial Time, TT(PPTA11).We successfully follow features known to affect the frequency of the TAI, and we find marginally significant differences between TT(PPTA11) and TT(BIPM11). We discuss the various phenomena that lead to a correlated signal in the pulsar timing residuals and therefore limit the stability of the pulsar time-scale.

Funding

Australian Research Council

European Commission

National Natural Science Foundation of China

Commonwealth Scientific and Industrial Research Organisation

History

Available versions

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ISSN

1365-2966

Journal title

Monthly Notices of the Royal Astronomical Society

Volume

427

Issue

4

Pagination

7 pp

Publisher

Wiley

Copyright statement

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2012 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Language

eng

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