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For astronomical applications is necessary to have high precision in sensing and processing the image data. In this time are used the large CCD sensors from the various reasons. For the replacement of CCD sensors with CMOS sensing devices is important to know transfer characteristics of used CCD sensors. In the special applications like the robotic telescopes (fully automatic, without human interactions) seems to be good using of specially designed smart sensors, which have integrated more functions and have more features than CCDs.
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Stanislav Vitek, "Measurement and analysis of image sensors," Proc. SPIE 5944, Smart Imagers and Their Application, 59440J (6 December 2006); https://doi.org/10.1117/12.637927