Background due to cosmic protons in gamma-ray telescopes
By: Henry L. Edwards.
Contributors: United States. National Aeronautics and Space Administration.
Series: NASA contractor report -- NASA/CR-186921.
Publisher: Stanford University, W.W. Hansen Experimental Physics Laboratory; National Aeronautics and Space Administration
Published: 1990
Place of publication: Stanford, Calif; [Washington, D.C
Language: eng
Format: Microform
Subjects: Calibrating.; Gamma ray astronomy.; Gamma ray telescopes.; Gamma rays.; Imaging techniques.; Monte Carlo method.; Protons.; Sensitivity.
Other titles: Study of the sensitivity of an imaging telescope (GRITS) for high energy gamma-ray astronomy.
Notes: "Final report"--Prelim. p.

Shipping list no.: 91-0428-M.

"June 6, 1990."

"August 1990"--Prelim. p.

Also available via Internet from the NASA Technical Report Server web site. Address as of 8/26/05: http://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/19900019152%5F1990019152.pdf; current access available via PURL.

Microfiche. [Washington, D.C. : National Aeronautics and Space Administration, 1990]. 1 microfiche. Header title: Study of the sensitivity of an imaging telescope (GRITS) for high energy gamma-ray astronomy.