English

Development of the ComPair gamma-ray telescope prototype

Instrumentation and Methods for Astrophysics 2022-10-07 v1 High Energy Astrophysical Phenomena Instrumentation and Detectors

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.

Keywords

Cite

@article{arxiv.2210.02962,
  title  = {Development of the ComPair gamma-ray telescope prototype},
  author = {Daniel Shy and Carolyn Kierans and Nicolas Cannady and Regina Caputo and Sean Griffin and J. Eric Grove and Elizabeth Hays and Emily Kong and Nicholas Kirschner and Iker Liceaga-Indart and Julie McEnery and John Mitchell and A. A. Moiseev and Lucas Parker and Jeremy S. Perkins and Bernard Phlips and Makoto Sasaki and Adam J. Schoenwald and Clio Sleator and Jacob Smith and Lucas D. Smith and Sambid Wasti and Richard Woolf and Eric Wulf and Anna Zajczyk},
  journal= {arXiv preprint arXiv:2210.02962},
  year   = {2022}
}
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