Characterization and optimization of MIT Lincoln Labs CCID20 CCDs

被引:11
作者
Wei, M [1 ]
Stover, RJ [1 ]
机构
[1] Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
来源
OPTICAL ASTRONOMICAL INSTRUMENTATION, PTS 1 AND 2 | 1998年 / 3355卷
关键词
CCD; characterization; optimization; high-resistivity; CCID20; MIT/Lincoln; UCO/Lick Observatory;
D O I
10.1117/12.316755
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
CCID20 CCDs are designed and produced by personnel at MIT/Lincoln Laboratory(1). The CCDs are thinned, back illuminated, 4096x2048 15-um square pixel, three-side buttable devices. Some CCDs have been made on high-resistivity bulk silicon and others have been made on standard resistivity epitaxial silicon. Recently many devices from the first round of production of these CCDs have been tested at the UCO/Lick Observatory Detector Development Laboratory. In this paper we present the results of the measurements of horizontal and vertical charge transfer efficiency, low-temperature dark current, localized charge traps, full well, responsive quantum efficiency, and fringing. We present performance measurements of the on-chip amplifier including measurements of read-out noise, gain and linearity with different bias voltages. Cross-talk between the two on-chip amplifiers is discussed. High resistivity CCDs made by MIT/Lincoln show higher QE and less QE variation at long wavelengths than regular thin CCDs. However, they are subject to additional lateral charge diffusion and cosmic-ray effects. We will give a comparison between the two kinds of CCID20 CCDs. CCID20 CCDs are not MPP devices. It is much more difficult to get high full well, low spurious charge, low dark current and low residual image, simultaneously. We present optimized parallel clocks and a special erasing procedure to help solve these problems. Devices from this first round of CCID20 CCDs exhibit a rectangular pattern of QE variations caused by backside surface treatment problems.
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页码:598 / 607
页数:2
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