The Anti-Coincidence Detector for the GLAST Large Area Telescope
arXiv:astro-ph/0702581 · doi:10.1016/j.astropartphys.2006.12.003
Abstract
This paper describes the design, fabrication and testing of the Anti-Coincidence Detector (ACD) for the Gamma-ray Large Area Space Telescope (GLAST) Large Area Telescope (LAT). The ACD is LAT first-level defense against the charged cosmic ray background that outnumbers the gamma rays by 3-5 orders of magnitude. The ACD covers the top and 4 sides of the LAT tracking detector, requiring a total active area of ~8.3 square meters. The ACD detector utilizes plastic scintillator tiles with wave-length shifting fiber readout. In order to suppress self-veto by shower particles at high gamma-ray energies, the ACD is segmented into 89 tiles of different sizes. The overall ACD efficiency for detection of singly charged relativistic particles entering the tracking detector from the top or sides of the LAT exceeds the required 0.9997.
33 pages, 19 figures
Cited by in corpus (9)
- Pre-launch estimates for GLAST sensitivity to Dark Matter annihilation signals
- Fermi Large Area Telescope Performance After 10 Years Of Operation
- Gamma-ray Astrophysics in the MeV Range: the ASTROGAM Concept and Beyond
- Massive Argon Space Telescope (MAST): a concept of heavy time projection chamber for gamma-ray astronomy in the 100 MeV --- 1 TeV energy range
- The GeV-TeV Connection in Galactic gamma-ray sources
- The e-ASTROGAM gamma-ray space mission
- Telescope Concepts in Gamma-Ray Astronomy
- Analysis Methods for Gamma-ray Astronomy
- The Fermi Large Area Telescope