Multi-messenger astronomy with INTEGRAL
C. Ferrigno, V. Savchenko, A. Coleiro, F. Panessa, A. Bazzano, E., Bozzo, J. Chenevez, A. Domingo, M. Doyle, A. Goldwurm, D. Goetz, E. Jourdain,, A. von Kienlin, E. Kuulkers, S. Mereghetti, A. Martin-Carrillo, L. Natalucci,, F. Onori, J. Rodi, J. Pierre Roques

TL;DR
INTEGRAL's versatile design enables it to contribute significantly to multi-messenger astronomy by detecting and constraining gamma-ray emissions associated with various cosmic phenomena like neutron star mergers, black hole binaries, and fast radio bursts.
Contribution
This paper reviews how INTEGRAL has uniquely contributed to multi-messenger astronomy through its observations and upper limits on gamma-ray emissions from diverse cosmic events.
Findings
Detected gamma-ray emission coincident with a neutron star merger.
Set upper limits on gamma-ray emissions from fast radio bursts.
Contributed to understanding the spectral energy distribution of a blazar linked to a neutrino event.
Abstract
At the time of defining the science objectives of the INTernational Gamma-Ray Astrophysics Laboratory (INTEGRAL), such a rapid and spectacular development of multi-messenger astronomy could not have been predicted, with new impulsive phenomena becoming accessible through different channels. Neutrino telescopes have routinely detected energetic neutrino events coming from unknown cosmic sources since 2013. Gravitational wave detectors opened a novel window on the sky in 2015 with the detection of the merging of two black holes and in 2017 with the merging of two neutron stars, followed by signals in the full electromagnetic range. Finally, since 2007, radio telescopes detected extremely intense and short burst of radio waves, known as Fast Radio Bursts (FRBs) whose origin is for most cases extragalactic, but enigmatic. The exceptionally robust and versatile design of the INTEGRAL…
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