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The position sensitive low energy detector on board the ZEBRA telescope
Authors:L Barbareschi  C La Padula  M Mastropietro  F Perotti  G Villa  A Bazzano  L Boccaccini  R Patriarca  VF Polcaro  P Ubertini  RC Butler  G Di Cocco  G Spada  JN Carter  P Charalambous  AJ Dean  JB Stephen
Institution:1. Istituto di Fisica Cosmica, CNR, Milano, Italy;7. Istituto di Astrofisica Spaziale, CNR, Frascati, Italy;71. Istituto TESRE/CNR, Bologna, Italy;77. University of Southampton, Southampton, UK
Abstract:In order to improve the low energy capability (15 ÷ 150 KeV) of the balloon borne “ZEBRA” low energy gamma imaging telescope (150 KeV-20 MeV), a large area, high spectral resolution (5% at 60 KeV), low background detector has been designed and is now under development.It consists of two MultiWire Spectroscopic Proportional Counter (SPC), escape gated, that have a sensitive area of 6000 cm2, and are placed above the large area array of sodiumiodide position sensitive elements.
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