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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.
Alexandre I. Baklanov,Victor I. Bogachev,Anatoly V. Yeltsov, andVjacheslav 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); https://doi.org/10.1117/12.238208
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Alexandre I. Baklanov, Victor I. Bogachev, Anatoly V. Yeltsov, 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); https://doi.org/10.1117/12.238208