Results from the CsI Calorimeter onboard the 2023 ComPair Balloon Flight

Daniel Shy,Richard S. Woolf,Clio Sleator,Bernard Phlips,J. Eric Grove,Eric A. Wulf, Mary Johnson-Rambert, Mitch Davis,Emily Kong, Thomas Caligiure, A. Wilder Crosier,Aleksey Bolotnikov,Nicholas Cannady,Gabriella A. Carini,Regina Caputo, Jack Fried, Priyarshini Ghosh,Sean Griffin,Elizabeth Hays,Sven Herrmann,Carolyn Kierans, Nicholas Kirschner, Iker Liceaga-Indart, Zachary Metzler,Julie McEnery,John Mitchell, A. A. Moiseev,Lucas Parker, Alfred Dellapenna,Jeremy S. Perkins,Makoto Sasaki, Adam J. Schoenwald, Lucas D. Smith,Janeth Valverde,Sambid Wasti, Anna Zajczyk

arxiv(2024)

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摘要
The ComPair gamma-ray telescope is a technology demonstrator for a future gamma-ray telescope called the All-sky Medium Energy Gamma-ray Observatory (AMEGO). The instrument is composed of four subsystems, a double-sided silicon strip detector, a virtual Frisch grid CdZnTe calorimeter, a CsI:Tl based calorimeter, and an anti-coincidence detector (ACD). The CsI calorimeter's goal is to measure the position and energy deposited from high-energy events. To demonstrate the technological readiness, the calorimeter has flown onboard a NASA scientific balloon as part of the GRAPE-ComPair mission and accumulated around 3 hours of float time at an altitude of 40 km. During the flight, the CsI calorimeter observed background radiation, Regener-Pfotzer Maximum, and several gamma-ray activation lines originating from aluminum.
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