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The Parkes Pulsar Timing Array project: second data release
Kerr, Matthew1; Reardon, Daniel J.2,3; Hobbs, George3,4; Shannon, Ryan M.2,3; Manchester, Richard N.4; Dai, Shi4; Russell, Christopher J.5; Zhang, Songbo4,6,7,8; van Straten, Willem9; Oslowski, Stefan2,3; Parthasarathy, Aditya2,3,4; Spiewak, Renee2,3; Bailes, Matthew2,3; Bhat, N. D. Ramesh10; Cameron, Andrew D.4; Coles, William A.11; Dempsey, James12; Deng, Xinping4; Goncharov, Boris3,13; Kaczmarek, Jane F.14; Keith, Michael J.15; Lasky, Paul D.3,13; Lower, Marcus E.2,3,4; Preisig, Brett14; Sarkissian, John Mihran14; Toomey, Lawrence4; Wang, Hongguang16; Wang, Jingbo17; Zhang, Lei4,6,18; Zhu, Xingjiang3,13
2020
Source PublicationPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
ISSN1323-3580
Volume37Pages:e020
Contribution Rank17
AbstractWe describe 14 yr of public data from the Parkes Pulsar Timing Array (PPTA), an ongoing project that is producing precise measurements of pulse times of arrival from 26 millisecond pulsars using the 64-m Parkes radio telescope with a cadence of approximately 3 weeks in three observing bands. A comprehensive description of the pulsar observing systems employed at the telescope since 2004 is provided, including the calibration methodology and an analysis of the stability of system components. We attempt to provide full accounting of the reduction from the raw measured Stokes parameters to pulse times of arrival to aid third parties in reproducing our results. This conversion is encapsulated in a processing pipeline designed to track provenance. Our data products include pulse times of arrival for each of the pulsars along with an initial set of pulsar parameters and noise models. The calibrated pulse profiles and timing template profiles are also available. These data represent almost 21 000 h of recorded data spanning over 14 yr. After accounting for processes that induce time-correlated noise, 22 of the pulsars have weighted root-mean-square timing residuals of <1 mu s in at least one radio band. The data should allow end users to quickly undertake their own gravitational wave analyses, for example, without having to understand the intricacies of pulsar polarisation calibration or attain a mastery of radio frequency interference mitigation as is required when analysing raw data files.
Keywordgravitational waves instrumentation: miscellaneous methods: observational pulsars: general
DOI10.1017/pasa.2020.11
URL查看原文
Indexed BySCI
Language英语
WOS KeywordRADIO ASTRONOMICAL POLARIMETRY ; CONTINUOUS GRAVITATIONAL-WAVES ; MILLISECOND PULSARS ; SOLAR-SYSTEM ; SPIN NOISE ; PRECISION ; LIMITS ; DISCOVERY ; BINARY ; DISPERSION
Funding ProjectNASA ; Australian Research Council grant[FL150100148] ; Australian Research Council[FT190100155] ; Australian Research Council[FT160100112] ; Australian Research Council[DP180103155] ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav)[CE170100004] ; National Natural Science Foundation of China[11573008] ; Youth Innovation Promotion Association of Chinese Academy of Sciences
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000538067000001
PublisherCAMBRIDGE UNIV PRESS
Funding OrganizationNASA ; Australian Research Council grant ; Australian Research Council ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav) ; National Natural Science Foundation of China ; Youth Innovation Promotion Association of Chinese Academy of Sciences
Citation statistics
Cited Times:31[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/3516
Collection射电天文研究室_脉冲星研究团组
Corresponding AuthorKerr, Matthew; Reardon, Daniel J.
Affiliation1.Naval Res Lab, Space Sci Div, Washington, DC 20375 USA
2.Swinburne Univ Technol, Ctr Astrophys & Supercomp, POB 218, Hawthorn, Vic 3122, Australia
3.Australian Res Council, Ctr Excellence Gravitat Wave Discovery OzGrav, Hawthorn, Vic, Australia
4.CSIRO Astron & Space Sci, Australia Telescope Natl Facil, POB 76, Epping, NSW 1710, Australia
5.CSIRO Sci Comp, Australian Technol Pk,Locked Bag 9013, Alexandria, NSW 1435, Australia
6.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
7.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
8.Univ Western Australia, Int Ctr Radio Astron Res, Crawley, WA 6009, Australia
9.Auckland Univ Technol, Inst Radio Astron & Space Res, Private Bag 92006, Auckland 1142, New Zealand
10.Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia
11.Univ Calif San Diego, Dept Elect & Comp Engn, La Jolla, CA 92093 USA
12.CSIRO Informat Management & Technol, GPO Box 1700, Canberra, ACT 2601, Australia
13.Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
14.CSIRO Astron & Space Sci, Parkes Observ, 473 Telescope Rd, Parkes, NSW 2870, Australia
15.Univ Manchester, Jodrell Bank Ctr Astrophys, Dept Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England
16.Guangzhou Univ, Sch Phys & Elect Engn, Guangzhou 510006, Peoples R China
17.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
18.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100101, Peoples R China
Recommended Citation
GB/T 7714
Kerr, Matthew,Reardon, Daniel J.,Hobbs, George,et al. The Parkes Pulsar Timing Array project: second data release[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA,2020,37:e020.
APA Kerr, Matthew.,Reardon, Daniel J..,Hobbs, George.,Shannon, Ryan M..,Manchester, Richard N..,...&Zhu, Xingjiang.(2020).The Parkes Pulsar Timing Array project: second data release.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA,37,e020.
MLA Kerr, Matthew,et al."The Parkes Pulsar Timing Array project: second data release".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA 37(2020):e020.
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