Calibration of the Energetic Gamma-Ray Experiment Telescope (egret) for the Compton Gamma-Ray Observatory

D. J. Thompson*, D. L. Bertsch, C. E. Fichtel, R. C. Hartman, R. Hofstadter, E. B. Hughes, S. D. Hunter, B. W. Hughlock, G. Kanbach, D. A. Kniffen, Y. C. Lin, J. R. Mattox, H. A. Mayer-Hasselwander, C. Von Montigny, P. L. Nolan, H. I. Nel, K. Pinkau, H. Rothermel, E. J. Schneid, M. SommerP. Sreekumar, D. Tieger, A. H. Walker

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

354 Citations (Scopus)

Abstract

Calibration of the Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma-Ray Observatory involves simulation, experimental calibration, and verification in flight. The principal properties of the instrument which have been determined as a function of energy and angle are the effective area, the angular resolution (point spread function), and the energy resolution (dispersion).

Original languageEnglish
Pages (from-to)629-656
Number of pages28
JournalAstrophysical Journal, Supplement Series
Volume86
Issue number2
DOIs
Publication statusPublished - 1993

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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