The observation of astrophysical objects in the mid-infrared requires Blocked Impurity Band (BIB) detectors based on n-doped Silicon. It is desirable to observe faint astronomical objects with such a detector, which can be achieved with a high signal to noise ratio. These detectors operate at a temp
β¦ LIBER β¦
Development of a cryogenic detection concept for GNO
β Scribed by Lanfranchi, J.-C; Lachenmaier, T; Potzel, W; von Feilitzsch, F
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 193 KB
- Volume
- 520
- Category
- Article
- ISSN
- 0168-9002
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