Development of the ComPair gamma-ray telescope prototype
arXiv:2210.02962 · doi:10.1117/12.2628811
Abstract
There is a growing interest in the science uniquely enabled by observations in the MeV range, particularly in light of multi-messenger astrophysics. The Compton Pair (ComPair) telescope, a prototype of the AMEGO Probe-class concept, consists of four subsystems that together detect and characterize gamma rays in the MeV regime. A double-sided strip silicon Tracker gives a precise measure of the first Compton scatter interaction and tracks pair-conversion products. A novel cadmium zinc telluride (CZT) detector with excellent position and energy resolution beneath the Tracker detects the Compton-scattered photons. A thick cesium iodide (CsI) calorimeter contains the high-energy Compton and pair events. The instrument is surrounded by a plastic anti-coincidence (ACD) detector to veto the cosmic-ray background. In this work, we will give an overview of the science motivation and a description of the prototype development and performance.
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Cited by in corpus (8)
- Detecting neutrino-boosted axion dark matter in the MeV gap
- Development of a CsI Calorimeter for the Compton-Pair (ComPair) Balloon-Borne Gamma-Ray Telescope
- Development of Dual-Gain SiPM Boards for Extending the Energy Dynamic Range
- Electromagnetic signatures of white dwarf collisions in AGN discs
- AstroPix: CMOS pixels in space
- Development of the cadmium zinc TElluride Radiation Imager (TERI)
- The 2023 Balloon Flight of the ComPair Instrument
- Background Measurements and Simulations of the ComPair Balloon Flight