Identifying multiwavelength counterparts to astrophysical neutrino events
arXiv:2309.06164 · doi:10.22323/1.444.1473
Abstract
High-energy neutrinos originating in astrophysical sources should be accompanied by gamma-rays at production. Depending on the properties of the emission environment and the distance of the source to the Earth, these gamma-rays may be observed directly, or through the detection of lower energy photons that result from interactions with the intervening radiation fields. In this work, we present an automated tool that aims at using data from the Fermi-Large Area Telescope to identify multiwavelength counterparts to astrophysical neutrino events. The main goal of this tool is to enable prompt follow-up observations with ground-based and space-based observatories in order to help pinpoint the neutrino source.
8 pages, 4 figures, Proceedings for the 38th International Cosmic Ray Conference (ICRC2023) in Nagoya, Japan. See https://multimessenger.ua.edu/fermi/ for webpage