[1] ANING Z, BLALOCK B J, ERICSON M N, et al. A high voltage CCD sensor control chip for the large synoptic survey telescope (LSST)[C]. IEEE Nuclear Science Symposium Conference Record, 2008: 2074-2078.
[2] DOHERTY P E, ANTILOGUS P, GILMORE D K, et al. Electro-optical testing of fully depleted CCD image sensors for the Large Synoptic Survey Telescope camera[C]. Proceedings of SPIE-The International Society for Optical Engineering, 2014, 9154(2): 38-39.
[3] XUE Yan-jie, XUE Sui-jian, ZHU Ming, et al. Overview of current status and development strategies in china′s astronomical facilities and related technologies[J]. Bulletin of Chinese Academy of Sciences, 2014(3): 368-375.
[4] ZHANG Yu-heng, YAN Yi-hua. Design of frame transfer area CCD imaging system for dark objects[J]. Acta Astronomica Sinica, 2015(3): 295-304
[5] WEI Ming-zhi, STOVER R J. New design for the UCO/Lick observatory CCD guide camera[C]. SPIE, 1996, 2654: 226-232.
[6] E2V Corporation.CCD203-82 back illuminated scientific CCD sensor data sheet[R]. 2005: 1-2
[7] CUI Xiang-qun, ZHAO Yong-heng, CHU Yao-quan, et al. The large sky area multi-object fiber spectroscopic telescope (LAMOST)[J].Research in Astronomy and Astrophysics, 2012, 12(9): 1197-1242.
[8] ZHAO Gang, ZHAO Yong-heng, CHU Yao-quan, et al. LAMOST spectral survey-an overview[J].Research in Astronomy and Astrophysics, 2012, 12(7): 723-734.
[9] E2V Corporation. CCD42-10 back illuminated high performance AIMO data sheet[R]. 2006: 1-2.