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A glitch in the millisecond pulsar J0613-0200

McKee, J. W.; Janssen, G. H.; Stappers, B. W.; Lyne, A. G.; Caballero, R. N.; Lentati, L.; Desvignes, G.; Jessner, A.; Jordan, C. A.; Karuppusamy, R.; Kramer, M.; Cognard, I.; Champion, D. J.; Graikou, E.; Lazarus, P.; Oslowski, S.; Perrodin, D.; Shaifullah, G.; Tiburzi, C.; Verbiest, J. P.W.

Authors

J. W. McKee

G. H. Janssen

B. W. Stappers

A. G. Lyne

R. N. Caballero

L. Lentati

G. Desvignes

A. Jessner

C. A. Jordan

R. Karuppusamy

M. Kramer

I. Cognard

D. J. Champion

E. Graikou

P. Lazarus

S. Oslowski

D. Perrodin

G. Shaifullah

C. Tiburzi

J. P.W. Verbiest



Abstract

We present evidence for a small glitch in the spin evolution of the millisecond pulsar J0613-0200, using the EPTA Data Release 1.0, combined with Jodrell Bank analogue filterbank times of arrival (TOAs) recorded with the Lovell telescope and Effelsberg Pulsar Observing System TOAs. A spin frequency step of 0.82(3) nHz and frequency derivative step of -1.6(39) × 10-19 Hz s-1 are measured at the epoch of MJD 50888(30). After PSR B1821-24A, this is only the second glitch ever observed in a millisecond pulsar, with a fractional size in frequency of δv/v = 2.5(1) × 10-12, which is several times smaller than the previous smallest glitch. PSR J0613-0200 is used in gravitational wave searches with pulsar timing arrays, and is to date only the second such pulsar to have experienced a glitch in a combined 886 pulsar-years of observations. We find that accurately modelling the glitch does not impact the timing precision for pulsar timing array applications. We estimate that for the current set of millisecond pulsars included in the International Pulsar Timing Array, there is a probability of ∼50 per cent that another glitch will be observed in a timing array pulsar within 10 years.

Citation

McKee, J. W., Janssen, G. H., Stappers, B. W., Lyne, A. G., Caballero, R. N., Lentati, L., Desvignes, G., Jessner, A., Jordan, C. A., Karuppusamy, R., Kramer, M., Cognard, I., Champion, D. J., Graikou, E., Lazarus, P., Oslowski, S., Perrodin, D., Shaifullah, G., Tiburzi, C., & Verbiest, J. P. (2016). A glitch in the millisecond pulsar J0613-0200. Monthly notices of the Royal Astronomical Society, 461(3), 2809-2817. https://doi.org/10.1093/mnras/stw1442

Journal Article Type Article
Acceptance Date Jun 13, 2016
Online Publication Date Jun 16, 2016
Publication Date Sep 21, 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 461
Issue 3
Pages 2809-2817
DOI https://doi.org/10.1093/mnras/stw1442
Public URL https://hull-repository.worktribe.com/output/4134735

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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.





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