Share Email Print
cover

Proceedings Paper

UCSD high-energy x-ray timing experiment cosmic ray particle anticoincidence detector
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

The HEXTE, part of the X-Ray Timing Explorer (XTE), is designed to make high sensitivity temporal and spectral measurements of X-rays with energies between 15 and 250 keV using NaI/CsI phoswich scintillation counters. To achieve the required sensitivity it is necessary to provide anticoincidence of charged cosmic ray particles incident upon the instrument, some of which interact to produce background X-rays. The proposed cosmic ray particle anticoincidence shield detector for HEXTE uses a novel design based on plastic scintillators and wavelength-shifter bars. It consists of five segments, each with a 7 mm thick plastic scintillator, roughly 50 cm x 50 cm in size, coupled to two wavelength-shifter bars viewed by 1/2 inch photomultiplier tubes. These segments are configured into a five-sided, box-like structure around the main detector system. Results of laboratory testing of a model segment, and calculations of the expected performance of the flight segments and particle anticoincidence detector system are presented to demonstrate that the above anticoincidence detector system satisfies its scientific requirements.

Paper Details

Date Published: 1 October 1991
PDF: 10 pages
Proc. SPIE 1549, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy II, (1 October 1991); doi: 10.1117/12.48338
Show Author Affiliations
Paul L. Hink, Univ. of California/San Diego (United States)
Richard E. Rothschild, Univ. of California/San Diego (United States)
Michael R. Pelling, Univ. of California/San Diego (United States)
Daniel R. MacDonald, Univ. of California/San Diego (United States)
Duane E. Gruber, Univ. of California/San Diego (United States)


Published in SPIE Proceedings Vol. 1549:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy II
Oswald H. W. Siegmund; Richard E. Rothschild, Editor(s)

© SPIE. Terms of Use
Back to Top