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Modeling nonstationary noise in pulsar timing array data analysis

Falxa, Mikel; Antoniadis, J.; Champion, D. J.; Cognard, I.; Desvignes, G.; Guillemot, L.; Hu, H.; Janssen, G.; Jawor, J.; Karuppusamy, R.; Keith, M. J.; Kramer, M.; Lackeos, K.; Liu, K.; McKee, J. W.; Perrodin, D.; Sanidas, S. A.; Shaifullah, G. M.; Theureau, G.

Authors

Mikel Falxa

J. Antoniadis

D. J. Champion

I. Cognard

G. Desvignes

L. Guillemot

H. Hu

G. Janssen

J. Jawor

R. Karuppusamy

M. J. Keith

M. Kramer

K. Lackeos

K. Liu

D. Perrodin

S. A. Sanidas

G. M. Shaifullah

G. Theureau



Abstract

Pulsar timing array (PTA) collaborations recently reported evidence for the presence of a gravitational wave background (GWB) in their datasets. The main candidate that is expected to produce such a GWB is the population of supermassive black hole binaries. Some analyses showed that the recovered signal may exhibit time-dependent properties, i.e., nonstationarity. In this paper, we propose an approximated nonstationary Gaussian process model obtained from the perturbation of stationary processes. The presented method is applied to the second data release of the European Pulsar Timing Array to search for nonstationary features in the GWB. We analyzed the data in different time slices and showed that the inferred properties of the GWB evolve with time. We find no evidence for such nonstationary behavior and the Bayes factor in favor of the latter is ℬNS 𝑆=1.5. We argue that the evolution of the GWB properties most likely comes from the improvement of the observation cadence with time and better characterization of the noise of individual pulsars. Such nonstationary GWB could also be produced by the leakage of nonstationary features in the noise of individual pulsars or by the presence of an eccentric single source.

Citation

Falxa, M., Antoniadis, J., Champion, D., Cognard, I., Desvignes, G., Guillemot, L., …Theureau, G. (2024). Modeling nonstationary noise in pulsar timing array data analysis. Physical Review D, 109(12), Article 123010. https://doi.org/10.1103/physrevd.109.123010

Journal Article Type Article
Acceptance Date May 6, 2024
Online Publication Date Jun 4, 2024
Publication Date Jun 15, 2024
Deposit Date Jun 17, 2024
Publicly Available Date Jun 17, 2024
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 109
Issue 12
Article Number 123010
DOI https://doi.org/10.1103/physrevd.109.123010
Public URL https://hull-repository.worktribe.com/output/4710962

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