The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
Creators: name: Antoniadis, J.
name: Arumugam, P.
name: Arumugam, S.
name: Babak, S.
name: Bagchi, M.
name: Nielsen, A. -S. Bak
name: Bassa, C. G.
name: Bathula, A.
name: Berthereau, A.
name: Bonetti, M.
name: Bortolas, E.
name: Brook, P. R.
name: Burgay, M.
name: Caballero, R. N.
name: Chalumeau, A.
name: Champion, D. J.
name: Chanlaridis, S.
name: Chen, S.
name: Cognard, I.
name: Dandapat, S.
name: Deb, D.
name: Desai, S.
name: Desvignes, G.
name: Dhanda-Batra, N.
name: Dwivedi, C.
name: Falxa, M.
name: Ferdman, R. D.
name: Franchini, A.
name: Gair, J. R.
name: Goncharov, B.
name: Gopakumar, A.
name: Graikou, E.
name: Grießmeier, J. -M.
name: Guillemot, L.
name: Guo, Y. J.
name: Gupta, Y.
name: Hisano, S.
name: Hu, H.
name: Iraci, F.
name: Izquierdo-Villalba, D.
name: Jang, J.
name: Jawor, J.
name: Janssen, G. H.
name: Jessner, A.
name: Joshi, B. C.
name: Kareem, F.
name: Karuppusamy, R.
name: Keane, E. F.
name: Keith, M. J.
name: Kharbanda, D.
name: Kikunaga, T.
name: Kolhe, N.
name: Kramer, M.
name: Krishnakumar, M. A.
name: Lackeos, K.
name: Lee, K. J.
name: Liu, K.
name: Liu, Y.
name: Lyne, A. G.
name: McKee, J. W.
name: Maan, Y.
name: Main, R. A.
name: Mickaliger, M. B.
name: Nitu, I. C.
name: Nobleson, K.
name: Paladi, A. K.
name: Parthasarathy, A.
name: Perera, B. B. P.
name: Perrodin, D.
name: Petiteau, A.
name: Porayko, N. K.
name: Possenti, A.
name: Prabu, T.
name: Leclere, H. Quelquejay
name: Rana, P.
name: Samajdar, A.
name: Sanidas, S. A.
name: Sesana, A.
name: Shaifullah, G.
name: Singha, J.
name: Speri, L.
name: Spiewak, R.
name: Srivastava, A.
name: Stappers, B. W.
name: Surnis, M.
name: Susarla, S. C.
name: Susobhanan, A.
name: Takahashi, K.
name: Tarafdar, P.
name: Theureau, G.
name: Tiburzi, C.
name: van der Wateren, E.
name: Vecchio, A.
name: Krishnan, V. Venkatraman
name: Verbiest, J. P. W.
name: Wang, J.
name: Wang, L.
name: Wu, Z.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: 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 $0.1\%$ ($\gtrsim 3σ$ 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.
description: 21 pages, 14 figures, 4 appendix figures, accepted for publication in A&amp;A