Community efforts in gamma-ray astrophysics: Insights from the GR SIG

The NASA Gamma Ray Science Interest Group (GR SIG) serves as a central hub and platform for the hard X-ray and gamma-ray astrophysics communities. It convenes monthly virtual meetings to discuss recent scientific results, technological progress, and current and future missions. Additionally, the group curates a list of technological requirements for future hard X-ray and gamma-ray missions and gathers community feedback to formulate recommendations for supporting the unique needs of these scientific communities, encompassing organizational aspects and scientific funding.

This presentation will provide an overview of the current activities of the GR SIG, highlighting the recent launch of the Future Innovations in Gamma-ray Science Analysis Group (FIG SAG) taskforce. We will also outline various avenues and opportunities for community involvement, empowering individuals to contribute actively to the evolution of hard X-ray and gamma-ray astrophysics.