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Pre-merger alert to detect the very-high-energy prompt emission from binary neutron-star mergers: Einstein Telescope and Cherenkov Telescope Array synergy
Biswajit Banerjee, Gor Oganesyan, Marica Branchesi +8
The current generation of very-high-energy ray (VHE; E above 30 GeV) detectors (MAGIC and H.E.S.S.) have recently demonstrated the ability to detect the afterglow emission…
Neutrino search from γ-ray bursts during the prompt and X-ray afterglow phases using 10 years of IceCube public data
Francesco Lucarelli, Gor Oganesyan, Teresa Montaruli +5
Neutrino emission from gamma-ray bursts (GRBs) has been sought for a long time, and stringent limits on the most accredited GRB emission models have been obtained from IceCube. Mul…
Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
Samuele Ronchini, Marica Branchesi, Gor Oganesyan +6
The Einstein Telescope (ET) is going to bring a revolution for the future of multi-messenger astrophysics. In order to detect the counterparts of binary neutron star (BNS) mergers…
Constrains on the physics of the prompt emission from a distant and energetic gamma-ray burst GRB 220101A
Alessio Mei, Gor Oganesyan, Anastasia Tsvetkova +6
The emission region of -ray bursts (GRBs) is poorly constrained. The uncertainty on the size of the dissipation site spans over 4 orders of magnitude (…