Paper
18 October 1996 High-energy Antimatter Telescope (HEAT): basic design and performance
Stephane Coutu, S. W. Barwick, A. Bhattacharyya, James J. Beatty, C. R. Bower, C. Chaput, G. De Nolfo, Don Ellithorpe, D. Ficenec, J. Knapp, D. M. Lowder, Steven Matthew McKee, Dietrich Mueller, J. A. Musser, S. L. Nutter, E. Schneider, Simon P. Swordy, K. K. Tang, Gregory Tarle, Andrew D. Tomasch, E. Torbet
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Abstract
The high-energy antimatter telescope (HEAT) instrument has been flown successfully by high-altitude balloon in 1994 and 1995, in a configuration optimized for the detection and identification of cosmic-ray electrons and positrons at energies from about 1 GeV up to 50 GeV and beyond. It consists of a two-coil superconducting magnet and a precision drift-tube tracking hodoscope, complemented with a time-of-flight system, a transition radiation detector and an electromagnetic shower counter. We review the design criteria for optimal e+/- detection and identification, and assess the instruments' performance and background rejection during its first two flights. We also review the adaptation of HEAT for measurements of high-energy cosmic- ray antiprotons and for isotopic composition studies.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephane Coutu, S. W. Barwick, A. Bhattacharyya, James J. Beatty, C. R. Bower, C. Chaput, G. De Nolfo, Don Ellithorpe, D. Ficenec, J. Knapp, D. M. Lowder, Steven Matthew McKee, Dietrich Mueller, J. A. Musser, S. L. Nutter, E. Schneider, Simon P. Swordy, K. K. Tang, Gregory Tarle, Andrew D. Tomasch, and E. Torbet "High-energy Antimatter Telescope (HEAT): basic design and performance", Proc. SPIE 2806, Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions, (18 October 1996); https://doi.org/10.1117/12.253971
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KEYWORDS
Electrons

Particles

Chromium

Spectroscopy

Electromagnetism

Sensors

Magnetism

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