Hard-X-Ray/Soft-γ-Ray Imaging Sensor Assembly for Astronomy
TBMG-3145
09/01/2008
- Content
An improved sensor assembly has been developed for astronomical imaging at photon energies ranging from 1 to 100 keV. The assembly includes a thallium-doped cesium iodide scintillator divided into pixels and coupled to an array of high-gain avalanche photodiodes (APDs). Optionally, the array of APDs can be operated without the scintillator to detect photons at energies below 15 keV. The array of APDs is connected to compact electronic readout circuitry that includes, among other things, 64 independent channels for detection of photons in various energy ranges, up to a maximum energy of 100 keV, at a count rate up to 3 kHz. The readout signals are digitized and processed by imaging software that performs "on-the-fly" analysis.
- Citation
- "Hard-X-Ray/Soft-γ-Ray Imaging Sensor Assembly for Astronomy," Mobility Engineering, September 1, 2008.