Speaker
Description
Space-based gamma-ray astronomy is a crucial tool for investigating extreme astrophysical phenomena and has played a key role in advancing our understanding of high-energy processes in the Universe. Gamma rays are deeply connected to gravitational waves, neutrinos, and cosmic rays, making them essential for multi-messenger astrophysics. As several current missions approach the end of their operational lifetimes, it is increasingly important to reassess the field’s scientific priorities and technical needs. The Future Innovations in Gamma-ray Science Analysis Group (FIG SAG) was formed to identify the key science drivers, required capabilities, and strategic priorities for gamma-ray astrophysics in the coming decades. In this presentation, I will provide an update on the group's progress and discuss opportunities for community engagement as we prepare a report for NASA Headquarters in 2025.
