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Nuclear Compton Telescope : ウィキペディア英語版
Nuclear Compton Telescope

The ''Nuclear Compton Telescope'' (NCT) is a balloon-borne Compton telescope to observe the gamma-ray sky in the energy range from a few hundred keV to several MeV. Its main goals are to improve the understanding of Galactic nucleosynthesis, gamma-ray bursts, supernovae, black holes, and more.
==Instrumentation==

The Compton telescope uses an array of twelve Germanium detectors with high spectral resolution to detect gamma rays. On its bottom half the detector is surrounded by a Bismuth germanate scintillator to shield it from atmospheric gamma rays. The telescope has an overall field of view (FOV) of 25% of the sky.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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