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| Content Provider | IEEE Xplore Digital Library |
|---|---|
| Author | Saha, S.K. |
| Copyright Year | 2009 |
| Description | Author affiliation: Indian Institute of Astrophysics, Bangalore - 560 034, India (Saha, S.K.) |
| Abstract | Astronomical observations are dependent on focal-plane instruments, and detectors continue to play a key role. The detector technology is evolving rather fast with the large-format CMOS and CCD array mosaics, electron-multiplying CCDs, electron-avalanche photodiode arrays, quantum-well IR photon detectors etc. However, the requirements of artifact-free photon shot noise limited images are the higher sensitivity, higher quantum efficiency, reduced noise that includes dark current, read-out and amplifier noise, smaller point-spread functions and higher spectral bandwidth, etc. One of the fastest growing applications is signal sensing, particularly wavefront sensing for adaptive optics and fringe tracking for interferometry. A few detectors that are being used in astronomical imaging are discussed in this talk. |
| Starting Page | 442 |
| Ending Page | 445 |
| File Size | 358088 |
| Page Count | 4 |
| File Format | |
| ISBN | 9781424448463 |
| Language | English |
| Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date | 2009-12-22 |
| Publisher Place | India |
| Access Restriction | Subscribed |
| Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subject Keyword | Infrared detectors Charge coupled devices Instruments Space technology Noise reduction CMOS image sensors CMOS technology Optical noise Photodiodes Sensor arrays |
| Content Type | Text |
| Resource Type | Article |
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