From the 5 of 283 papers with an AI index.
23 citations
- Université Paris-SaclayFR121 papers
- Sapienza University of RomeIT115 papers
- Jagiellonian UniversityPL114 papers
- The Ohio State UniversityUS114 papers
- University of BolognaIT114 papers
- University of GenoaIT114 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di GenovaIT113 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT112 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT112 papers
- LIP - Laboratory of Instrumentation and Experimental Particle PhysicsPT112 papers
- European Organization for Nuclear ResearchCH111 papers
- AGH University of KrakowPL110 papers
8 papers · 1 filter
Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes
K. Abe, S. Abe, J. Abhir +439
We present very-high-energy gamma-ray observations of two binary black hole merger candidates, GW240615_113620 and GW241125_010116, performed with the Major Atmospheric Gamma Imagi…
Constraining gamma-ray burst parameters with the first ultra-high energy neutrino event KM3-230213A
KM3NeT Collaboration, O. Adriani, A. Albert +278
Context: The detection of the highest energy neutrino observed to date by KM3NeT, with an estimated energy of 220 PeV, opens up new possibilities for the study and identification o…
Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
S. Abe, J. Abhir, A. Abhishek +457
The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), together with its electromagnetic counterpart, th…
Quantifying the impact of relativistic precession on tidal disruption event light curves
Diego Calderón, OndÅej Pejcha, Brian D. Metzger +2
The tidal field of a black hole can turn a star into a gas stream whose orbit can precess, especially if the a black hole is rapidly spinning. In this work, we investigate the impa…
Search for ultra-high energy neutrons from Galactic sources with the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Abdul Halim, P. Abreu +357
Deflections in the propagation of charged ultra-high-energy cosmic rays (UHECRs) caused by magnetic fields make the identification of their sources challenging. On the other hand,…
Tomographic constraints on the high-energy cosmic neutrino emission rate
Alberto Gálvez Ureña, Federico Urban, David Alonso
Despite growing efforts to find the sources of high energy neutrinos measured by IceCube, the bulk of the neutrinos remain with unknown origins. We aim to constrain the emissivity…