_version_ 1866910462709334016
author Shy, Daniel
Woolf, Richard S.
Sleator, Clio
Phlips, Bernard
Grove, J. Eric
Wulf, Eric A.
Johnson-Rambert, Mary
Davis, Mitch
Kong, Emily
Caligiure, Thomas
Crosier, A. Wilder
Bolotnikov, Aleksey
Cannady, Nicholas
Carini, Gabriella A.
Caputo, Regina
Fried, Jack
Ghosh, Priyarshini
Griffin, Sean
Hays, Elizabeth
Herrmann, Sven
Kierans, Carolyn
Kirschner, Nicholas
Liceaga-Indart, Iker
Metzler, Zachary
McEnery, Julie
Mitchell, John
Moiseev, A. A.
Parker, Lucas
Dellapenna, Alfred
Perkins, Jeremy S.
Sasaki, Makoto
Schoenwald, Adam J.
Smith, Lucas D.
Valverde, Janeth
Wasti, Sambid
Zajczyk, Anna
author_facet Shy, Daniel
Woolf, Richard S.
Sleator, Clio
Phlips, Bernard
Grove, J. Eric
Wulf, Eric A.
Johnson-Rambert, Mary
Davis, Mitch
Kong, Emily
Caligiure, Thomas
Crosier, A. Wilder
Bolotnikov, Aleksey
Cannady, Nicholas
Carini, Gabriella A.
Caputo, Regina
Fried, Jack
Ghosh, Priyarshini
Griffin, Sean
Hays, Elizabeth
Herrmann, Sven
Kierans, Carolyn
Kirschner, Nicholas
Liceaga-Indart, Iker
Metzler, Zachary
McEnery, Julie
Mitchell, John
Moiseev, A. A.
Parker, Lucas
Dellapenna, Alfred
Perkins, Jeremy S.
Sasaki, Makoto
Schoenwald, Adam J.
Smith, Lucas D.
Valverde, Janeth
Wasti, Sambid
Zajczyk, Anna
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2405_06839
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Results from the CsI Calorimeter onboard the 2023 ComPair Balloon Flight
Shy, Daniel
Woolf, Richard S.
Sleator, Clio
Phlips, Bernard
Grove, J. Eric
Wulf, Eric A.
Johnson-Rambert, Mary
Davis, Mitch
Kong, Emily
Caligiure, Thomas
Crosier, A. Wilder
Bolotnikov, Aleksey
Cannady, Nicholas
Carini, Gabriella A.
Caputo, Regina
Fried, Jack
Ghosh, Priyarshini
Griffin, Sean
Hays, Elizabeth
Herrmann, Sven
Kierans, Carolyn
Kirschner, Nicholas
Liceaga-Indart, Iker
Metzler, Zachary
McEnery, Julie
Mitchell, John
Moiseev, A. A.
Parker, Lucas
Dellapenna, Alfred
Perkins, Jeremy S.
Sasaki, Makoto
Schoenwald, Adam J.
Smith, Lucas D.
Valverde, Janeth
Wasti, Sambid
Zajczyk, Anna
Instrumentation and Methods for Astrophysics
Nuclear Experiment
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.
title Results from the CsI Calorimeter onboard the 2023 ComPair Balloon Flight
topic Instrumentation and Methods for Astrophysics
Nuclear Experiment
url https://arxiv.org/abs/2405.06839