Ponente
Descripción
Galactic sources are key to understanding cosmic-ray acceleration and the extreme astrophysics environment in the Milky Way. Some of these sources are expected to emit both gamma rays and neutrinos: while gamma rays trace high-energy particle interactions, neutrinos provide a direct probe of hadronic acceleration processes. To study these phenomena, observatories with broad energy coverage and high-duty cycles, such as KM3NeT and HAWC, are particularly well-suited. Both instruments are optimized for time-integrated observations and can also support follow-up studies of transient events. In this work, we present first estimations of the capabilities of a joint KM3NeT and HAWC analysis to constrain the hadronic contribution to the emission processes of selected Galactic sources, using KM3NeT Monte Carlo simulations and HAWC observational data. The analysis is performed within the Gammapy framework, enabling a unified treatment of gamma-ray and neutrino data with consistent modeling and likelihood fitting.
