Gamma ray observations in the energy range 0.3&lt;E&lt;5.0 GeV from balloons

Sood, R. K.; Clayton, P. G.; Roff, C. E.; Hughes, J. B.; Rochester, G. K.

doi:10.1088/0022-3735/15/4/017

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Lower Time Ol Flight -Spark Chamber -Calorimeter1

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1987

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“…1985, Sood et al 1982). In common with detectors at other energies, considerable effort is put into maximising angular and energy resolution without loss of detection efficiency.…”

Section: Lower Time Ol Flight -Spark Chamber -Calorimetermentioning

confidence: 99%

Gamma-Ray Astronomy From Balloons and Satellites (Invited Paper)

Sood

1987

Publ. Astron. Soc. Aust.

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Gamma-ray astronomy has traditionally been a difficult field of research due to the low fluxes from astronomical objects and the inherently poor angular response of detectors. Progress made in the field in the last twenty years is reviewed. Many major astrophysical problems can only be addressed with the future operation of more sensitive satellite experiments. Recent gamma-ray observations of the supernova SN1987 a are briefly discussed.

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“…1985, Sood et al 1982). In common with detectors at other energies, considerable effort is put into maximising angular and energy resolution without loss of detection efficiency.…”

Section: Lower Time Ol Flight -Spark Chamber -Calorimetermentioning

confidence: 99%