Paper
24 April 1995 Ultraviolet detectors for astrophysics: present and future
Melville P. Ulmer, Manijeh Razeghi, Erwan Bigan
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Abstract
Astronomical instruments for the study of UV astronomy have been developed for NASA missions such as the Hubble Space Telescope. The systems that are `blind to the visible' (`solar-blind') yet sensitive to the UV that have been flown in satellites have detective efficiencies of about 10 to 20%, although typically electron bombardment charge coupled devices are higher at 30 - 40% and ordinary CCDs achieve 1 - 5%. Therefore, there is a large payoff still to be gained by further improvements in the performance of solar blind UV detectors. We provide a brief review of some aspects of UV astronomy, UV detector development, and possible technologies for the future. We suggest that a particularly promising future technology is one based on the ability of investigators to produce high quality films made of wide bandgap III-V semiconductors.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Melville P. Ulmer, Manijeh Razeghi, and Erwan Bigan "Ultraviolet detectors for astrophysics: present and future", Proc. SPIE 2397, Optoelectronic Integrated Circuit Materials, Physics, and Devices, (24 April 1995); https://doi.org/10.1117/12.206870
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Cited by 39 scholarly publications.
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KEYWORDS
Ultraviolet radiation

Sensors

Charge-coupled devices

Ultraviolet astronomy

Astronomy

Galactic astronomy

Imaging spectroscopy

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