K. Liu
Variability, polarimetry, and timing properties of single pulses from PSR J1713+0747 using the Large European Array for Pulsars
Liu, K.; Bassa, C. G.; Janssen, G. H.; Karuppusamy, R.; McKee, J.; Kramer, M.; Lee, K. J.; Perrodin, D.; Purver, M.; Sanidas, S.; Smits, R.; Stappers, B. W.; Weltevrede, P.; Zhu, W. W.
Authors
C. G. Bassa
G. H. Janssen
R. Karuppusamy
J. McKee
M. Kramer
K. J. Lee
D. Perrodin
M. Purver
S. Sanidas
R. Smits
B. W. Stappers
P. Weltevrede
W. W. Zhu
Abstract
Single pulses preserve information about the pulsar radio emission and propagation in the pulsar magnetosphere, and understanding the behaviour of their variability is essential for estimating the fundamental limit on the achievable pulsar timing precision. Here we report the findings of our analysis of single pulses from PSR J1713+0747 with data collected by the Large European Array for Pulsars (LEAP). We present statistical studies of the pulse properties that include distributions of their energy, phase and width. Two modes of systematic sub-pulse drifting have been detected, with a periodicity of seven and three pulse periods. The two modes appear at different ranges of pulse longitude but overlap under the main peak of the integrated profile. No evidence for pulse micro-structure is seen with a time resolution down to 140 ns. In addition, we show that the fractional polarization of single pulses increases with their pulse peak flux density. By mapping the probability density of linear polarization position angle with pulse longitude, we reveal the existence of two orthogonal polarization modes. Finally, we find that the resulting phase jitter of integrated profiles caused by single pulse variability can be described by a Gaussian probability distribution only when at least 100 pulses are used for integration. Pulses of different flux densities and widths contribute approximately equally to the phase jitter, and no improvement on timing precision is achieved by using a sub-set of pulses with a specific range of flux density or width.
Citation
Liu, K., Bassa, C. G., Janssen, G. H., Karuppusamy, R., McKee, J., Kramer, M., Lee, K. J., Perrodin, D., Purver, M., Sanidas, S., Smits, R., Stappers, B. W., Weltevrede, P., & Zhu, W. W. (2016). Variability, polarimetry, and timing properties of single pulses from PSR J1713+0747 using the Large European Array for Pulsars. Monthly notices of the Royal Astronomical Society, 463(3), 3239-3248. https://doi.org/10.1093/mnras/stw2223
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 1, 2016 |
Online Publication Date | Sep 5, 2016 |
Publication Date | Dec 11, 2016 |
Deposit Date | Nov 29, 2022 |
Publicly Available Date | Feb 17, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 463 |
Issue | 3 |
Pages | 3239-3248 |
DOI | https://doi.org/10.1093/mnras/stw2223 |
Public URL | https://hull-repository.worktribe.com/output/4134728 |
Files
Published article
(3.3 Mb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2016 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
Modeling nonstationary noise in pulsar timing array data analysis
(2024)
Journal Article
NANOGrav 15-year gravitational-wave background methods
(2024)
Journal Article
Downloadable Citations
About Repository@Hull
Administrator e-mail: repository@hull.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search