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Instrument description and performance of the Imaging Gamma-Ray Telescope COMPTEL aboard the Compton Gamma-Ray Observatory

Authors :
G. Stacy
H. Aarts
M. Kippen
J. Clear
R. Much
J. A. Lockwood
K. Bennett
C. Winkler
Derek W. Morris
L. Kuiper
C. de Vries
W. Hermsen
A. Deerenberg
M. Snelling
G. G. Lichti
J. W. den Herder
B. G. Taylor
Mark L. McConnell
Werner Collmar
Roland Diehl
A. Connors
B. N. Swanenburg
James M. Ryan
H. de Boer
Andrew W. Strong
Helmut Steinle
Volker Schoenfelder
G. Simpson
J. R. Macri
A. von Dordrecht
Source :
Astrophysical Journal Supplement Series, Astrophysical Journal Supplement Series, 86, 657-692. University of Chicago Press
Publication Year :
1993

Abstract

The imaging Compton telescope COMPTEL is one of the four instruments on board the Compton Gamma-Ray Observatory (GRO), which was launched on 1991 April 5 by the space shuttle Atlantis into an Earth orbit of 450 km altitude. COMPTEL is exploring the 1-30 MeV energy range with an angular resolution (1σ) between 1° and 2° within a large field of view of about 1 steradian. Its energy resolution (8.8% FWHM at 1.27 MeV) makes it a powerful gamma-ray line spectrometer. Its effective area (for on-axis incidence) varies between 10 and 50 cm 2 depending on energy and event selections. Within a 14 day observation period COMPTEL is able to detect sources which are about 20 times weaker than the Crab. The measurement principle of COMPTEL also allows the measurements of solar neutrons

Details

Language :
English
Database :
OpenAIRE
Journal :
Astrophysical Journal Supplement Series, Astrophysical Journal Supplement Series, 86, 657-692. University of Chicago Press
Accession number :
edsair.doi.dedup.....632303a1e532cbbbd4998429304cf5b7