Molecular beam epitaxial mercury cadmium telluride: A quiet, warm FPA for NGST

被引：0
|
作者：
Hall, DNB [1 ]
Hodapp, KW [1 ]
Goldsmith, DL [1 ]
Cabelli, CA [1 ]
Cooper, DE [1 ]
Montroy, JT [1 ]
Pasko, JG [1 ]
Vural, K [1 ]
Zandian, M [1 ]
机构：
[1] Univ Hawaii, Astron Inst, Honolulu, HI 96822 USA
来源：
NGST SCIENCE AND TECHNOLOGY EXPOSITION | 2000年 / 207卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In a 1K x 1K FPA utilizing 4.8 mu m MBE HCT, over 97% of pixels exhibit dark current similar to 0.01 e(-)/sec and multiple sampled read noise similar to 4 e(-) at a temperature of 64 K and bias of 200 mV. These correspond to a total noise of 5 e(-) in 1,000 seconds, intermediate between the NGST requirement of 10 e(-) and the goal of 3 e(-).
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页码：79 / 83
页数：3
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