- By:
- Moiseev, Alex; Gonzalez, Francisco M; Steinhebel, Amanda L; Ziock, Klaus-Peter
- Page Number:
- 765
- Volume:
- 501
- Book Title:
- Proceedings of the 39th International Cosmic Ray Conference (ICRC2025) - Gamma-Ray Astrophysics
- Publication Date:
- March 12, 2026
- Publisher Location:
- Proceedings of Science, United States of America
- Conference Name:
- 39th International Cosmic Ray Conference (ICRC2025)
- Conference Location:
- Geneva, Switzerland
- Conference Sponsor:
- NASA
- View DOI Listing:
- https://doi.org/10.22323/1.501.0765
Abstract
The Galactic Annihilation Line Explorer (GALE) mission will address the long-standing question of the sources of Galactic positrons: whether they are produced by unresolved astrophysical sources or created via diffuse processes, possibly due to dark matter decay and/or annihilation. The problem of Galactic positrons that produce 511-keV gamma-ray emission from the Galactic plane and Galactic Center has existed for years and is well-defined by the measurements of INTEGRAL/SPI. GALE is designed to achieve the needed angular resolution (fraction of a degree) and point source sensitivity (< 10−4 ph/cm2/s) required to understand the 511-keV emission structure in the Galactic Center. The GALE instrument combines a coded-aperture mask (CAM) with a cadmium-zinc-telluride imaging calorimeter (ImCal) to form a combined CAM/Compton telescope. This is mated with the Wallops Arc-Second Pointer (WASP) support system to achieve the precise telescope pointing control required for imaging the Galactic Center. In this paper, the science goals, GALE instrument concept, anticipated performance and mission results will be discussed.
