Abstract
We have developed a low noise, low power charge sensitive amplifier and pulse shaping circuit. Our application is for a double-sided germanium strip detector, nominally providing 50 independent spectroscopy channels. An array of these detectors would provide significant improvements in imaging, spectroscopy and sensitivity for space-based gamma-ray astronomy. The key features of these electronics are low noise, very low power, and a small footprint per channel. Performance of our first circuit is in good agreement with simulations, with ~205e noise rms (0 pF), and 3 mW/channel power consumption. Dynamic range is 0–3.3 MeV (germanium) with a linearity of ±0.6%. Performance of this prototype device will be discussed.
| Original language | English |
|---|---|
| Pages (from-to) | 921-924 |
| Number of pages | 4 |
| Journal | IEEE Transactions on Nuclear Science |
| Volume | 42 |
| Issue number | 4 |
| DOIs | |
| State | Published - Aug 1995 |
Funding
*This work was supported in part by the Office of Naval Research and NASA, under contract No. W-18486.
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