D. Shy, C. Kierans, N. Cannady, R. Caputo, S. Griffin, E. Grove, E. Hays, E. Kong, N. Kirschner, I. Liceaga-Indart, J. Mcenery, J. Mitchell, A. Moiseev, L. Parker, J. Perkins, B. Phlips, M. Sasaki, Adam J. Schoenwald, C. Sleator, J. Smith, L. Smith, S. Wasti, R. Woolf, E. Wulf, A. Zajczyk
{"title":"Development of the ComPair gamma-ray telescope prototype","authors":"D. Shy, C. Kierans, N. Cannady, R. Caputo, S. Griffin, E. Grove, E. Hays, E. Kong, N. Kirschner, I. Liceaga-Indart, J. Mcenery, J. Mitchell, A. Moiseev, L. Parker, J. Perkins, B. Phlips, M. Sasaki, Adam J. Schoenwald, C. Sleator, J. Smith, L. Smith, S. Wasti, R. Woolf, E. Wulf, A. Zajczyk","doi":"10.1117/12.2628811","DOIUrl":null,"url":null,"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.","PeriodicalId":137463,"journal":{"name":"Astronomical Telescopes + Instrumentation","volume":"32 16","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-08-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"6","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomical Telescopes + Instrumentation","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2628811","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 6
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.