In-flight calibration of EGRET on the Compton Gamma-Ray Observatory

J. A. Esposito*, D. L. Bertsch, A. W. Chen, B. L. Dingus, C. E. Fichtel, R. C. Hartman, S. D. Hunter, G. Kanbach, D. A. Kniffen, Y. C. Lin, H. A. Mayer-Hasselwander, L. M. Mcdonald, P. F. Michelson, C. Von Montigny, R. Mukherjee, P. L. Nolan, O. L. Reimer, E. Schneid, P. Sreekumar, D. J. ThompsonW. F. Tompkins, T. D. Willis

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

66 Citations (Scopus)

Abstract

The Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma-Ray Observatory has been operating for over 7 yr since its launch in 1991 April. This span of time far exceeds the design lifetime of 2 yr. As the instrument has aged, several changes have occurred owing to spark chamber gas exchanges as well as some hardware degradation and failures, all of which have an influence on the instrument sensitivity. This paper describes postlaunch measurements and analysis that are done to cali-brate the instrument response functions. The updated instrument characteristics are incorporated into the analysis software.

Original languageEnglish
Pages (from-to)203-217
Number of pages15
JournalAstrophysical Journal, Supplement Series
Volume123
Issue number1
DOIs
Publication statusPublished - 07-1999

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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