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High-resolution imaging : detectors and applications /
Interferometric observations need snapshots of very high time resolution of the order of (i) frame integration of about 100 Hz or (ii) photon-recording rates of several megahertz (MHz). Detectors play a key role in astronomical observations, and since the explanation of the photoelectric effect by A...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
[Singapore] :
Pan Stanford Publishing,
[2015]
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| Temas: | |
| Acceso en línea: | Texto completo Texto completo |
MARC
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| 100 | 1 | |a Saha, Swapan K., |e author. | |
| 245 | 1 | 0 | |a High-resolution imaging : |b detectors and applications / |c Swapan K. Saha. |
| 264 | 1 | |a [Singapore] : |b Pan Stanford Publishing, |c [2015] | |
| 264 | 4 | |c ©2015 | |
| 300 | |a 1 online resource (xxxiii, 565 pages) : |b illustrations | ||
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| 504 | |a Includes bibliographical references and index. | ||
| 588 | 0 | |a Online resource; title from PDF title page (CRCnetBASE, viewed on March 10, 2015). | |
| 505 | 0 | |a Properties of Radiation -- Photoelectric Concept -- Concept of Laser -- Photon Detection Process -- Photodetectors -- Charge Transfer Devices -- Photon-Counting Systems -- Radiation Detectors for Infrared Wavelengths. | |
| 520 | |a Interferometric observations need snapshots of very high time resolution of the order of (i) frame integration of about 100 Hz or (ii) photon-recording rates of several megahertz (MHz). Detectors play a key role in astronomical observations, and since the explanation of the photoelectric effect by Albert Einstein, the technology has evolved rather fast. The present-day technology has made it possible to develop large-format complementary metal oxide-semiconductor (CMOS) and charge-coupled device (CCD) array mosaics, orthogonal transfer CCDs, electron-multiplication CCDs, electron-avalanche photodiode arrays, and quantum-well infrared (IR) photon detectors. The requirements to develop artifact-free photon shot noise-limited images are higher sensitivity and quantum efficiency, reduced noise that includes dark current, read-out and amplifier noise, smaller point-spread functions, and higher spectral bandwidth. This book aims to address such systems, technologies and design, evaluation and calibration, control electronics, scientific applications, and results. | ||
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