Institutional Repository of Radio Astronomy Research Laboratory
Effect of Matching Algorithm and Profile Shape on Pulsar Pulse Time of Arrival Uncertainties | |
Wang, J.1,2,3![]() ![]() | |
2023-12-01 | |
Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
![]() |
ISSN | 1674-4527 |
Volume | 23Issue:12Pages:125020 |
Contribution Rank | 8 |
Abstract | For high-precision pulsar timing analysis and low-frequency gravitational wave detection, it is essential to accurately determine pulsar pulse times of arrival (ToAs) and associated uncertainties. To measure the ToAs and their uncertainties, various cross-correlation-based techniques can be employed. We develop methodologies to investigate the impact of the template-matching method, profile shape, signal-to-noise ratio of both template and observation on ToA uncertainties. These methodologies are then applied to data from the International Pulsar Timing Array. We demonstrate that the Fourier domain Markov chain Monte Carlo method is generally superior to other methods, while the Gaussian interpolation shift method outperforms other methods in certain cases, such as profiles with large duty cycles or smooth profiles without sharp features. However, it is important to note that our study focuses solely on ToA uncertainty, and the optimal method for determining both ToA and ToA uncertainty may differ. |
Keyword | methods: data analysis (stars:) pulsars: general methods: statistical |
DOI | 10.1088/1674-4527/ad013d |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | PRECISION |
Funding Project | We would like to express our gratitude to J. -M. Grieszlig ; meier for providing valuable suggestions. Additionally, we extend our thanks to the anonymous RAA referees for offering constructive feedback to enhance the quality of the article. J. P. W. V. ack[433075039] ; Deutsche Forschungsgemeinschaft (DFG) through the Heisenberg program |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:001105359800001 |
Publisher | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
Funding Organization | We would like to express our gratitude to J. -M. Grieszlig ; meier for providing valuable suggestions. Additionally, we extend our thanks to the anonymous RAA referees for offering constructive feedback to enhance the quality of the article. J. P. W. V. ack ; Deutsche Forschungsgemeinschaft (DFG) through the Heisenberg program |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/5596 |
Collection | 射电天文研究室_脉冲星研究团组 |
Corresponding Author | Wang, J. |
Affiliation | 1.Ruhr Univ Bochum, Astron Inst AIRUB, Fak Phys & Astron, D-44801 Bochum, Germany 2.Beijing Normal Univ, Adv Inst Nat Sci, Zhuhai 519087, Peoples R China 3.Univ Bielefeld, Fak Phys, Postfach 100131, D-33501 Bielefeld, Germany 4.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany 5.Univ Cent Florida, Florida Space Inst, 12354 Res Pkwy, Orlando, FL 32826 USA 6.Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy 7.Ist Nazl Fis Nucl, Sez Milano Bicocca, Piazza Sci 3, I-20126 Milan, Italy 8.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 9.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China 10.INAF Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargius, CA, Italy |
Recommended Citation GB/T 7714 | Wang, J.,Verbiest, J. P. W.,Shaifullah, G. M.,et al. Effect of Matching Algorithm and Profile Shape on Pulsar Pulse Time of Arrival Uncertainties[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2023,23(12):125020. |
APA | Wang, J.,Verbiest, J. P. W.,Shaifullah, G. M.,&Yuan, J. P..(2023).Effect of Matching Algorithm and Profile Shape on Pulsar Pulse Time of Arrival Uncertainties.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,23(12),125020. |
MLA | Wang, J.,et al."Effect of Matching Algorithm and Profile Shape on Pulsar Pulse Time of Arrival Uncertainties".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 23.12(2023):125020. |
Files in This Item: | ||||||
File Name/Size | DocType | Version | Access | License | ||
Wang-2023-Effect of (5990KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment