The Parkes Pulsar Timing Array third data release

A. Zic; D. J. Reardon; A. Kapur; G. Hobbs; R. Mandow; M. Curyło; R. M. Shannon; J. Askew; M. Bailes; N. D. Ramesh Bhat; A. Cameron; Z. C. Chen; Shi Dai; V. Di Marco; Y. Feng; M. Kerr; A. Kulkarni; M. E. Lower; R. Luo; R. N. Manchester; M. T. Miles; R. S. Nathan; S. Osłowski; A. F. Rogers; C. J. Russell; R. Spiewak; N. Thyagarajan; L. Toomey; S. Wang; L. Zhang; S. Zhang; X. J. Zhu

doi:10.1017/pasa.2023.36

The Parkes Pulsar Timing Array third data release

A. Zic
, D. J. Reardon
, A. Kapur
, G. Hobbs
, R. Mandow
, M. Curyło
, R. M. Shannon
, J. Askew
, M. Bailes
, N. D. Ramesh Bhat
, A. Cameron
, Z. C. Chen
, Shi Dai
, V. Di Marco
, Y. Feng
, M. Kerr
, A. Kulkarni
, M. E. Lower
, R. Luo
, R. N. Manchester

M. T. Miles, R. S. Nathan, S. Osłowski, A. F. Rogers, C. J. Russell, R. Spiewak, N. Thyagarajan, L. Toomey, S. Wang, L. Zhang, S. Zhang, X. J. Zhu

Western Sydney University

Research output: Contribution to journal › Article › peer-review

186 Citations (Scopus)

Abstract

We present the third data release from the Parkes Pulsar Timing Array (PPTA) project. The release contains observations of 32 pulsars obtained using the 64-m Parkes "Murriyang"radio telescope. The data span is up to 18 years with a typical cadence of 3 weeks. This data release is formed by combining an updated version of our second data release with âˆ¼3 years of more recent data primarily obtained using an ultra-wide-bandwidth receiver system that operates between 704 and 4032 MHz. We provide calibrated pulse profiles, flux-density dynamic spectra, pulse times of arrival, and initial pulsar timing models. We describe methods for processing such wide-bandwidth observations, and compare this data release with our previous release.

Original language	English
Article number	e049
Number of pages	12
Journal	Publications of the Astronomical Society of Australia
Volume	40
DOIs	https://doi.org/10.1017/pasa.2023.36
Publication status	Published - 2023

Keywords

Gravitational wave astronomy (675)
Millisecond pulsars (1062)
Gravitational waves (678)
Pulsar timing method (1305)

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10.1017/pasa.2023.36

Cite this

Zic, A., Reardon, D. J., Kapur, A., Hobbs, G., Mandow, R., Curyło, M., Shannon, R. M., Askew, J., Bailes, M., Ramesh Bhat, N. D., Cameron, A., Chen, Z. C., Dai, S., Di Marco, V., Feng, Y., Kerr, M., Kulkarni, A., Lower, M. E., Luo, R., ... Zhu, X. J. (2023). The Parkes Pulsar Timing Array third data release. Publications of the Astronomical Society of Australia, 40, Article e049. https://doi.org/10.1017/pasa.2023.36

@article{13558c6809614e7b8b31edd0bfbae2bc,

title = "The Parkes Pulsar Timing Array third data release",

abstract = "We present the third data release from the Parkes Pulsar Timing Array (PPTA) project. The release contains observations of 32 pulsars obtained using the 64-m Parkes {"}Murriyang{"}radio telescope. The data span is up to 18 years with a typical cadence of 3 weeks. This data release is formed by combining an updated version of our second data release with {\^a}ˆ¼3 years of more recent data primarily obtained using an ultra-wide-bandwidth receiver system that operates between 704 and 4032 MHz. We provide calibrated pulse profiles, flux-density dynamic spectra, pulse times of arrival, and initial pulsar timing models. We describe methods for processing such wide-bandwidth observations, and compare this data release with our previous release.",

keywords = "Gravitational wave astronomy (675), Millisecond pulsars (1062), Gravitational waves (678), Pulsar timing method (1305)",

author = "A. Zic and Reardon, \{D. J.\} and A. Kapur and G. Hobbs and R. Mandow and M. Cury{\l}o and Shannon, \{R. M.\} and J. Askew and M. Bailes and \{Ramesh Bhat\}, \{N. D.\} and A. Cameron and Chen, \{Z. C.\} and Shi Dai and \{Di Marco\}, V. and Y. Feng and M. Kerr and A. Kulkarni and Lower, \{M. E.\} and R. Luo and Manchester, \{R. N.\} and Miles, \{M. T.\} and Nathan, \{R. S.\} and S. Os{\l}owski and Rogers, \{A. F.\} and Russell, \{C. J.\} and R. Spiewak and N. Thyagarajan and L. Toomey and S. Wang and L. Zhang and S. Zhang and Zhu, \{X. J.\}",

year = "2023",

doi = "10.1017/pasa.2023.36",

language = "English",

volume = "40",

journal = "Publications of the Astronomical Society of Australia",

issn = "1323-3580",

publisher = "CSIRO",

}

Zic, A, Reardon, DJ, Kapur, A, Hobbs, G, Mandow, R, Curyło, M, Shannon, RM, Askew, J, Bailes, M, Ramesh Bhat, ND, Cameron, A, Chen, ZC, Dai, S, Di Marco, V, Feng, Y, Kerr, M, Kulkarni, A, Lower, ME, Luo, R, Manchester, RN, Miles, MT, Nathan, RS, Osłowski, S, Rogers, AF, Russell, CJ, Spiewak, R, Thyagarajan, N, Toomey, L, Wang, S, Zhang, L, Zhang, S & Zhu, XJ 2023, 'The Parkes Pulsar Timing Array third data release', Publications of the Astronomical Society of Australia, vol. 40, e049. https://doi.org/10.1017/pasa.2023.36

TY - JOUR

T1 - The Parkes Pulsar Timing Array third data release

AU - Zic, A.

AU - Reardon, D. J.

AU - Kapur, A.

AU - Hobbs, G.

AU - Mandow, R.

AU - Curyło, M.

AU - Shannon, R. M.

AU - Askew, J.

AU - Bailes, M.

AU - Ramesh Bhat, N. D.

AU - Cameron, A.

AU - Chen, Z. C.

AU - Dai, Shi

AU - Di Marco, V.

AU - Feng, Y.

AU - Kerr, M.

AU - Kulkarni, A.

AU - Lower, M. E.

AU - Luo, R.

AU - Manchester, R. N.

AU - Miles, M. T.

AU - Nathan, R. S.

AU - Osłowski, S.

AU - Rogers, A. F.

AU - Russell, C. J.

AU - Spiewak, R.

AU - Thyagarajan, N.

AU - Toomey, L.

AU - Wang, S.

AU - Zhang, L.

AU - Zhang, S.

AU - Zhu, X. J.

PY - 2023

Y1 - 2023

N2 - We present the third data release from the Parkes Pulsar Timing Array (PPTA) project. The release contains observations of 32 pulsars obtained using the 64-m Parkes "Murriyang"radio telescope. The data span is up to 18 years with a typical cadence of 3 weeks. This data release is formed by combining an updated version of our second data release with âˆ¼3 years of more recent data primarily obtained using an ultra-wide-bandwidth receiver system that operates between 704 and 4032 MHz. We provide calibrated pulse profiles, flux-density dynamic spectra, pulse times of arrival, and initial pulsar timing models. We describe methods for processing such wide-bandwidth observations, and compare this data release with our previous release.

AB - We present the third data release from the Parkes Pulsar Timing Array (PPTA) project. The release contains observations of 32 pulsars obtained using the 64-m Parkes "Murriyang"radio telescope. The data span is up to 18 years with a typical cadence of 3 weeks. This data release is formed by combining an updated version of our second data release with âˆ¼3 years of more recent data primarily obtained using an ultra-wide-bandwidth receiver system that operates between 704 and 4032 MHz. We provide calibrated pulse profiles, flux-density dynamic spectra, pulse times of arrival, and initial pulsar timing models. We describe methods for processing such wide-bandwidth observations, and compare this data release with our previous release.

KW - Gravitational wave astronomy (675)

KW - Millisecond pulsars (1062)

KW - Gravitational waves (678)

KW - Pulsar timing method (1305)

UR - https://hdl.handle.net/1959.7/uws:73526

UR - https://www.scopus.com/pages/publications/85165950011

U2 - 10.1017/pasa.2023.36

DO - 10.1017/pasa.2023.36

M3 - Article

SN - 1323-3580

VL - 40

JO - Publications of the Astronomical Society of Australia

JF - Publications of the Astronomical Society of Australia

M1 - e049

ER -

The Parkes Pulsar Timing Array third data release

Abstract

Keywords

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