Tracing Out The Neutrino Sky With TAMBO

Argüelles C.A.; Bazo J.; Briceño C.; Bustamante M.; Carbajal S.; Centa V.; de Swart J.; Delgado D.; Dorigo T.; Fedynitch A.; Fernández P.; Gago A.; García A.; Giuffra A.; Hampel-Arias Z.; Kheirandish A.; Lazar J.P.; Lewis P.M.; Menéndez D.; Milla M.; Peláez A.; Romero-Wolf A.; Safa I.; Stucchi L.; Tarrillo J.; Thompson W.G.; Vischia P.; Vincent A.C.; Zhelnin P. · Proceedings of Science (2025) · DOI: 10.22323/1.501.0981

Resumen

Traditional searches for neutrino point sources have been hindered by the look-elsewhere effect. To address this, TAMBO will generate a catalog of neutrino source localizations - each localization equivalent in size to the square of TAMBO’s angular resolution. In doing so, TAMBO will have significantly reduced the available space to be searched by neutrino observatories, thus decreasing the trials factor necessary to elevate a local significance to a global one. In this talk we will present projected sensitivities to various neutrino sources and the effect of a TAMBO event to neutrino source discovery in IceCube. By refining the search through precise source localizations, TAMBO enhances the detection capabilities of observatories like IceCube, paving the way for efficient identification and confirmation of neutrino sources. © Copyright owned by the author(s)

Instituciones: Pontificia Universidad Católica del Perú; Universidad del Pacífico; Universidad de Ingeniería y Tecnología