Infrared and Laser Engineering, Volume. 52, Issue 12, 20230316(2023)
Study on performance testing techniques for astronomical optical cameras
Fig. 2. The four main processes of CMOS are completed in one pixel[11]
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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