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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  V.F. Polcaro  P. Ubertini  R.C. Butler  G. Di Cocco  G. Spada  J.N. Carter  P. Charalambous  A.J. Dean  J.B. Stephen
Affiliation: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.
Keywords:
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