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  The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

Antoniadis, J., Arumugam, P., Arumugam, S., Babak, S., Bagchi, M., Nielsen, A.-.-S.-B., et al. (2023). The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals. Astronomy and Astrophysics, 678: A50. doi:10.1051/0004-6361/202346844.

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Antoniadis, J., Author
Arumugam, P., Author
Arumugam, S., Author
Babak, S., Author
Bagchi, M., Author
Nielsen, A. -S. Bak, Author
Bassa, C. G., Author
Bathula, A., Author
Berthereau, A., Author
Bonetti, M., Author
Bortolas, E., Author
Brook, P. R., Author
Burgay, M., Author
Caballero, R. N., Author
Chalumeau, A., Author
Champion, D. J., Author
Chanlaridis, S., Author
Chen, S., Author
Cognard, I., Author
Dandapat, S., Author
Deb, D., AuthorDesai, S., AuthorDesvignes, G., AuthorDhanda-Batra, N., AuthorDwivedi, C., AuthorFalxa, M., AuthorFerdman, R. D., AuthorFranchini, A., AuthorGair, J. R.1, Author           Goncharov, B., AuthorGopakumar, A., AuthorGraikou, E., AuthorGrießmeier, J. -M., AuthorGuillemot, L., AuthorGuo, Y. J., AuthorGupta, Y., AuthorHisano, S., AuthorHu, H., AuthorIraci, F., AuthorIzquierdo-Villalba, D., AuthorJang, J., AuthorJawor, J., AuthorJanssen, G. H., AuthorJessner, A., AuthorJoshi, B. C., AuthorKareem, F., AuthorKaruppusamy, R., AuthorKeane, E. F., AuthorKeith, M. J., AuthorKharbanda, D., AuthorKikunaga, T., AuthorKolhe, N., AuthorKramer, M., AuthorKrishnakumar, M. A., AuthorLackeos, K., AuthorLee, K. J., AuthorLiu, K., AuthorLiu, Y., AuthorLyne, A. G., AuthorMcKee, J. W., AuthorMaan, Y., AuthorMain, R. A., AuthorMickaliger, M. B., AuthorNitu, I. C., AuthorNobleson, K., AuthorPaladi, A. K., AuthorParthasarathy, A., AuthorPerera, B. B. P., AuthorPerrodin, D., AuthorPetiteau, A., AuthorPorayko, N. K., AuthorPossenti, A., AuthorPrabu, T., AuthorLeclere, H. Quelquejay, AuthorRana, P., AuthorSamajdar, A., AuthorSanidas, S. A., AuthorSesana, A., AuthorShaifullah, G., AuthorSingha, J., AuthorSperi, L.1, Author           Spiewak, R., AuthorSrivastava, A., AuthorStappers, B. W., AuthorSurnis, M., AuthorSusarla, S. C., AuthorSusobhanan, A., AuthorTakahashi, K., AuthorTarafdar, P., AuthorTheureau, G., AuthorTiburzi, C., Authorvan der Wateren, E., AuthorVecchio, A., AuthorKrishnan, V. Venkatraman, AuthorVerbiest, J. P. W., AuthorWang, J., AuthorWang, L., AuthorWu, Z., Author more..
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

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Free keywords: Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO, Astrophysics, Galaxy Astrophysics, astro-ph.GA
 Abstract: We present the results of the search for an isotropic stochastic
gravitational wave background (GWB) at nanohertz frequencies using the second
data release of the European Pulsar Timing Array (EPTA) for 25 millisecond
pulsars and a combination with the first data release of the Indian Pulsar
Timing Array (InPTA). We analysed (i) the full 24.7-year EPTA data set, (ii)
its 10.3-year subset based on modern observing systems, (iii) the combination
of the full data set with the first data release of the InPTA for ten commonly
timed millisecond pulsars, and (iv) the combination of the 10.3-year subset
with the InPTA data. These combinations allowed us to probe the contributions
of instrumental noise and interstellar propagation effects. With the full data
set, we find marginal evidence for a GWB, with a Bayes factor of four and a
false alarm probability of $4\%$. With the 10.3-year subset, we report evidence
for a GWB, with a Bayes factor of $60$ and a false alarm probability of about
$0.1\%$ ($\gtrsim 3\sigma$ significance). The addition of the InPTA data yields
results that are broadly consistent with the EPTA-only data sets, with the
benefit of better noise modelling. Analyses were performed with different data
processing pipelines to test the consistency of the results from independent
software packages. The inferred spectrum from the latest EPTA data from new
generation observing systems is rather uncertain and in mild tension with the
common signal measured in the full data set. However, if the spectral index is
fixed at 13/3, the two data sets give a similar amplitude of
($2.5\pm0.7)\times10^{-15}$ at a reference frequency of $1\,{\rm yr}^{-1}$. By
continuing our detection efforts as part of the International Pulsar Timing
Array (IPTA), we expect to be able to improve the measurement of spatial
correlations and better characterise this signal in the coming years.

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 Dates: 2023-06-282023
 Publication Status: Issued
 Pages: 21 pages, 14 figures, 4 appendix figures, accepted for publication in A&A
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 2306.16214
DOI: 10.1051/0004-6361/202346844
 Degree: -

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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 678 Sequence Number: A50 Start / End Page: - Identifier: -