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The application of two-dimensional imaging to very high energy gamma ray astronomy. [Smithsonian Institution Astrophysical Observatory, Cambridge, Massachusetts]

Technical Report ·
DOI:https://doi.org/10.2172/6874099· OSTI ID:6874099
After an introductory overview of gamma-ray astronomy, very brief summaries of research results are given. Summary topics may be grouped as follows: observations (survey of candidate gamma-ray sources; Cygnus X-3; Markarian 421; AGN's: general survey; Crab observations: pulsar outburst; Geminga; AE Aqr; bursts; ARTEMIS; muon telescope), technical developments (11m telescope: dedication and performance; 10m mount control; CCD cameras; light cones; filters; GRANITE upgrade; trigger configuration; miror coatings; lightning protection), data analysis (quick look; optical disk archive; false source method), infrastructure, and reviews.
Research Organization:
Smithsonian Institution, Cambridge, MA (United States). Smithsonian Astrophysical Observatory
Sponsoring Organization:
DOE; NASA; USDOE, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States)
DOE Contract Number:
FG02-91ER40635
OSTI ID:
6874099
Report Number(s):
DOE/ER/40635-1; ON: DE93012326
Country of Publication:
United States
Language:
English