[1] J. Janesick,F. Gunaman,T. Dosluoglu et al.. Scientific CMOS pixels[C]. Conf. Proc. on Scientific Detectors for Astronomy,2004,300:103-114
[2] Orly Yadid-Pecht,Ralph Etienne-Cummings. CMOS Imagers:From Phototransduction to Image Processing[M]. Dordrecht:Kluwer Academic Publishers,2004
[3] Y. Shang,Y. Guan,W. Zhang et al.. A high dynamic range complementary metal-oxide-semiconductor (CMOS) camera using multi-slope response and an image reconstruction algorithm[J]. Meas. Sci. Technol.,2009,10( ):104002
[4] M. R. Stanford,B. J Hadwen. The noise performance of electron multiplying charge coupled devices[J]. IEEE Trans. Electron. Devices,2003,50(5):1227-1232
[5] H. Tian,Boyd Fowler,Abbas El Gamal. Analysis of temporal noise in CMOS photodiode active pixel sensor[J]. IEEE J. Solid-State Circuits,2001,36(1):92-100
[6] Y. Shang,J. Zhang,Y. Guan et al.. Design and evaluation of a high-performance CCD (charge coupled device) camera for astronomical imaging[J]. Meas. Sci. Technol.,2009,20(10):104005
[7] Song Qian. Radiation Damage on the Charge-Coupled Devices Used in Space Astronomical Obervatory[D]. Kunming:Yunnan Astronomical Observatory Chinese Academy of Sciences,2002
[8] Cypress Company. LUPA-4000 4 M Pixel CMOS Image Sensor Specification[R]. January,2007
[9] B. Ye,Q. Song. How accurate are the QE measurements[C]. Conf. Proc. On Scientific Detectors for Astronomy,2004,300:511-514