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Article Dans Une Revue Astrophys.J. Année : 2018

Coincident detection significance in multimessenger astronomy

G. Ashton
  • Fonction : Auteur
E. Burns
  • Fonction : Auteur
T.Dal Canton
T. Dent
  • Fonction : Auteur
H.-B Eggenstein
  • Fonction : Auteur
A.B. Nielsen
  • Fonction : Auteur
R. Prix
  • Fonction : Auteur
M. Was
S.J. Zhu
  • Fonction : Auteur

Résumé

We derive a Bayesian criterion for assessing whether signals observed in two separate data sets originate from a common source. The Bayes factor for a common versus unrelated origin of signals includes an overlap integral of the posterior distributions over the common-source parameters. Focusing on multimessenger gravitational-wave astronomy, we apply the method to the spatial and temporal association of independent gravitational-wave and electromagnetic (or neutrino) observations. As an example, we consider the coincidence between the recently discovered gravitational-wave signal GW170817 from a binary neutron star merger and the gamma-ray burst GRB 170817A: we find that the common-source model is enormously favored over a model describing them as unrelated signals.

Dates et versions

hal-01815325 , version 1 (14-06-2018)

Identifiants

Citer

G. Ashton, E. Burns, T.Dal Canton, T. Dent, H.-B Eggenstein, et al.. Coincident detection significance in multimessenger astronomy. Astrophys.J., 2018, 860 (1), pp.6. ⟨10.3847/1538-4357/aabfd2⟩. ⟨hal-01815325⟩
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