Infrared and Laser Engineering, Volume. 52, Issue 12, 20230316(2023)
Study on performance testing techniques for astronomical optical cameras
Fig. 1. Schematic diagram of FFCCD structure[6]
Fig. 2. The four main processes of CMOS are completed in one pixel[11]
Fig. 3. Schematic diagram of a CMOS[12]
Fig. 4. (a) Marana sCMOS;(b) iKon-L 936 CCD
Fig. 5. Set up of test platform in an optical dark room
Fig. 6. PTC of Marana sCMOS camera in the 12-bit setting
Fig. 7. PTC of iKon-L 936 CCD camera in the 1 MHz 4× setting
Fig. 8. Linearity curve of Marana sCMOS camera in the 12-bit setting
Fig. 9. Linearity curve of iKon-L 936 CCD camera in the 1 MHz 4× setting
Fig. 10. Time series samples of bias counts of the sCMOS camera in the 12-bit (a) and the CCD camera in the 1 MHz 4× (b) settings
Fig. 11. Histograms of number density of pixel RN measured with the sCMOS camera in the 12-bit (a) and the iKon-L CCD camera in the 1 MHz 4× (b) settings
Fig. 12. Changes in dark images obtained with the sCMOS camera in the 12-bit setting
Fig. 13. Changes in dark images obtained with the CCD camera in 1 MHz 4× the setting
Fig. 14. Dark current obtained with the sCMOS camera in the 12-bit (a) and CCD camera in the 1 MHz 4× setting (b)
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Peng Qiu, Sicheng Zou, Xiaoming Zhang, Jianfeng Wang, Qin Lin, Xiaojun Jiang. Study on performance testing techniques for astronomical optical cameras[J]. Infrared and Laser Engineering, 2023, 52(12): 20230316
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Received: May. 29, 2023
Accepted: --
Published Online: Feb. 23, 2024
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