The Structure of the ZEBRA Telescope, the Integration Tests and the First Calibration Results

Abstract
The ZEBRA telescope is a balloon borne low energy gamma ray instrument, sensitive in the photon energy range 0.2-10MeV. The main characteristics and components of the telescope are described, and its performance during laboratory calibration is discussed, after its integration with the flight electronics.

This publication has 3 references indexed in Scilit: