8 April 1996 Sensitivity of an optoelectronic CCD camera for astronomy
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Proceedings Volume 2790, Fifth Conference on Charge-Coupled Devices and CCD Systems; (1996) https://doi.org/10.1117/12.238208
Event: Fifth Conference on Charge-Coupled Devices and CCD Systems, 1995, Krym, Russian Federation
Abstract
An optoelectronic CCD camera for astronomy with a digital 10-bit output is described. A very high power objective is incorporated into the camera. The camera sensitivity is analyzed for radiation from stars of various spectra. The output signal is shown to be strongly dependent on a light source spectrum. Possible application are described.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alexandre I. Baklanov, Alexandre I. Baklanov, Victor I. Bogachev, Victor I. Bogachev, Anatoly V. Yeltsov, Anatoly V. Yeltsov, Vjacheslav V. Kolotkov, Vjacheslav V. Kolotkov, "Sensitivity of an optoelectronic CCD camera for astronomy", Proc. SPIE 2790, Fifth Conference on Charge-Coupled Devices and CCD Systems, (8 April 1996); doi: 10.1117/12.238208; https://doi.org/10.1117/12.238208
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