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Upper limits to pulsed gamma ray emission from PSR 0833-45, 1747-46, and 1818-04Pulsed gamma ray emission from three pulsars (PSR 0833-45, 1747-46, and 1818-04) have been sought on a balloon flight of the University of New Hampshire Large Gamma Ray Telescope, which incorporates a shielded sodium iodide scintillator array, and was launched from Alice Springs, Australia. Over the energy range 0.1 - 10 MeV, no evidence is found for pulsed gamma rays, and upper limits are set for Vela which are comparable to, or below, the extrapolation to lower energies of the pulsed emission reported by SAS-2 and COS-B.
Document ID
19820046846
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Cherry, M. L.
(Pennsylvania, University Philadelphia, PA, United States)
Dunphy, P. P.
(Pennsylvania Univ. Philadelphia, PA, United States)
Chupp, E. L.
(Pennsylvania Univ. Philadelphia, PA, United States)
Forrest, D. J.
(Pennsylvania Univ. Philadelphia, PA, United States)
Ryan, J. M.
(New Hampshire, University Durham, NH, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Subject Category
Astronomy
Meeting Information
Meeting: International Cosmic Ray Conference
Location: Paris
Country: France
Start Date: July 13, 1981
End Date: July 25, 1981
Accession Number
82A30381
Funding Number(s)
CONTRACT_GRANT: NGL-30-002-021
Distribution Limits
Public
Copyright
Other

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