Published June 21, 2007 | Version v1
Journal article

A study of the LXeGRIT detection efficiency for MeV gamma-rays during the 2000 balloon flight campaign

  • 1. Columbia Astrophysics Laboratory, Columbia University, New York, NY (United States) and Yale University, New Haven, CT (United States)
  • 2. Columbia Astrophysics Laboratory, Columbia University, New York, NY (United States)
  • 3. Waseda University, Tokyo (Japan)
  • 4. Department of Physics and Astronomy, Rice University, Houston, TX (United States)

Description

LXeGRIT-Liquid Xenon Gamma-Ray Imaging Telescope-is the first prototype of a Compton telescope (CT) for MeV γ-ray astrophysics based on a LXe time projection chamber. One of the most relevant figures of merit for a CT is the detection efficiency for γ-rays, which depends on diverse contributions such as detector geometry and passive materials, trigger efficiency, dead time, etc. A detailed study of the efficiency of the LXeGRIT instrument, based both on laboratory measurements and Monte Carlo (MC) simulations, is presented in this paper

Additional details

Identifiers

DOI
10.1016/j.nima.2007.02.102;
arXiv
arXiv:physics/0702078v2;
PII
S0168-9002(07)00417-2;

Publishing Information

Journal Title
Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
Journal Volume
576
Journal Issue
2-3
Journal Page Range
p. 350-361
ISSN
0168-9002
CODEN
NIMAER

Optional Information

Copyright
Copyright (c) 2007 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.