A pulsar-based time-scale from the International Pulsar Timing Array

@article{Hobbs2019APT,
  title={A pulsar-based time-scale from the International Pulsar Timing Array},
  author={George Hobbs and L. Guo and R. N. Caballero and W. A. Coles and K. J. Lee and Richard N. Manchester and Daniel J. Reardon and Demetrios N. Matsakis and Ming-lei Tong and Zaven Arzoumanian and Matthew Bailes and C. G. Bassa and N. D. Ramesh Bhat and Adam Brazier and Sarah Burke-Spolaor and David J. Champion and Sourav Chatterjee and Ismael Cognard and Shi Dai and Gregory Desvignes and Timothy Dolch and Robert D. Ferdman and Eleni Graikou and Lucas Guillemot and G. Janssen and Michael J. Keith and Matthew Kerr and Michael Kramer and Michael T. Lam and K. Liu and Andrew G. Lyne and T. Joseph W. Lazio and Ryan S. Lynch and James W. McKee and Maura Mclaughlin and Chiara M. F. Mingarelli and David J. Nice and Stefan Osłowski and Timothy T. Pennucci and Benetge B. P. Perera and D. Perrodin and Andrea Possenti and Christopher J. Russell and Sotiris Sanidas and Alberto Sesana and G M Shaifullah and Ryan M. Shannon and Joseph Simon and Ren{\'e}e Spiewak and Ingrid H. Stairs and Ben W. Stappers and Joseph K. Swiggum and S. R. Taylor and Gilles Theureau and Lawrence Toomey and R van Haasteren and J. B. Wang and Y. Wang and X J Zhu},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2019}
}
  • G. HobbsL. Guo X. Zhu
  • Published 30 October 2019
  • Physics
  • Monthly Notices of the Royal Astronomical Society
We have constructed a new time-scale, TT(IPTA16), based on observations of radio pulsars presented in the first data release from the International Pulsar Timing Array (IPTA). We used two analysis techniques with independent estimates of the noise models for the pulsar observations and different algorithms for obtaining the pulsar time-scale. The two analyses agree within the estimated uncertainties and both agree with TT(BIPM17), a post-corrected time-scale produced by the Bureau… 

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