The Darkest EMCCD ever

被引:18
作者
Daigle, Olivier [1 ,2 ]
Quirion, Pierre-Olivier [3 ]
Lessard, Simon [4 ]
机构
[1] Nuvu Cameras, 5155 Decelles Ave,Pavillon JA Bombardier, Montreal, PQ H3T 2B1, Canada
[2] Univ Montreal, Dept Phys, Expt Astrophys Lab, CP 6128, Montreal, PQ H3C 3J7, Canada
[3] Canadian Space Agcy, Montreal, PQ J3Y 8Y9, Canada
[4] Photon etc, Montreal, PQ H2S2X3, Canada
来源
HIGH ENERGY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY IV | 2010年 / 7742卷
关键词
Astronomical instrumentation; EMCCD; L3CCD; CIC; IPCS;
D O I
10.1117/12.856405
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
EMCCDs are devices capable of sub-electron read-out noise at high pixel rate, together with a high quantum efficiency (QE). However, they are plagued by an excess noise factor (ENF) which has the same effect on photometric measurement as if the QE would be halved. In order to get rid of the ENF, the photon counting (PC) operation is mandatory, with the drawback of counting only one photon per pixel per frame. The high frame rate capability of the EMCCDs comes to the rescue, at the price of increased clock induced charges (CIC), which dominates the noise budget of the EMCCD. The CIC can be greatly reduced with an appropriate clocking, which renders the PC operation of the EMCCD very efficient for faint flux photometry or spectroscopy, adaptive optics, ultrafast imaging and Lucky Imaging. This clocking is achievable with a new EMCCD controller: CCCP, the CCD Controller for Counting Photons. This new controller, which is now commercialized by Nuvu cameras inc., was integrated into an EMCCD camera and tested at the observatoire du mont-Megantic. The results are presented in this paper.
引用
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页数:11
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