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A liquid xenon imaging telescope for gamma ray astrophysics: Design and expected performanceA high resolution telescope for imaging cosmic x ray sources in the MeV region, with an angular resolution better than 0.5 deg is being developed as balloon-borne payload. The instrument consists of a 3-D liquid xenon TPC as x ray detector, coupled with a coded aperture at a distance of 1 meter. A study of the actual source distribution of the 1.809 MeV line from the decay of Al-26 and the 511 keV positron-electron annihilation line is among the scientific objectives, along with a search for new x ray sources. The telescope design parameters and expected minimum flux sensitivity to line and continuum radiation are presented. The unique capablity of the LXe-TPC as a Compton Polarimeter is also discussed.
Document ID
19930006402
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Aprile, E.
(Columbia Univ. New York, NY, United States)
Mukherjee, R.
(Columbia Univ. New York, NY, United States)
Chen, D.
(Columbia Univ. New York, NY, United States)
Bolotnikov, A.
(Columbia Univ. New York, NY, United States)
Date Acquired
September 6, 2013
Publication Date
December 1, 1992
Publication Information
Publication: Development of a High Resolution Liquid Xenon Imaging Telescope for Medium Energy Gamma Ray Astrophysics
Subject Category
Astronomy
Meeting Information
Meeting: International Conference on Advanced Technology and Particle Physics
Location: Como
Country: Italy
Start Date: June 22, 1992
End Date: June 26, 1992
Accession Number
93N15591
Funding Number(s)
CONTRACT_GRANT: NAGW-2013
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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