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Physical Review D

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Likelihoods for stochastic gravitational wave background data analysis

Gabriele Franciolini1,*, Mauro Pieroni1,2,†, Angelo Ricciardone3,4,‡, and Joseph D. Romano5,§

  • 1CERN, Theoretical Physics Department, Esplanade des Particules 1, Geneva 1211, Switzerland
  • 2Instituto de Estructura de la Materia (IEM), CSIC, Serrano 121, 28006 Madrid, Spain
  • 3Dipartimento di Fisica “Enrico Fermi”, Università di Pisa, Largo Bruno Pontecorvo 3, Pisa I-56127, Italy
  • 4INFN, Sezione di Pisa, Largo Bruno Pontecorvo 3, Pisa I-56127, Italy
  • 5Department of Physics and Astronomy, University of Texas Rio Grande Valley, One West University Boulevard, Brownsville, Texas 78520, USA

  • *Contact author: gabriele.franciolini@cern.ch
  • †Contact author: mauro.pieroni@csic.es
  • ‡Contact author: angelo.ricciardone@unipi.it
  • §Contact author: joseph.romano@utrgv.edu

Cosmic Variance in Anisotropy Searches at Pulsar Timing Arrays

Valerie Domcke, Gabriele Franciolini, and Mauro Pieroni

Phys. Rev. Lett. 137 061003 (2026)

Upper limits on the isotropic gravitational-wave background from the first part of LIGO, Virgo, and KAGRA’s fourth observing run

A. G. Abac et al.

Phys. Rev. D 114 042001 (2026)

Detectability and parameter estimation for Einstein Telescope configurations with GWJulia

Andrea Begnoni, Stefano Anselmi, Mauro Pieroni, Alessandro Renzi, and Angelo Ricciardone

J. Cosmol. Astropart. Phys. 2026 079 (2026)

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