Characterization of 2.5 micron HgCdTe VIRGO/VISTA detector array
Characterization of 2.5 micron HgCdTe VIRGO/VISTA detector array
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2.5 微米 HgCdTe VIRGO/VISTA 探测器阵列的表征
DOI：
10.1117/12.617789
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发表时间：
2005
期刊：
影响因子：
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通讯作者：
J. Pipher
中科院分区：
文献类型：
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作者：
C. McMurtry;T. Allen;A. Moore;W. Forrest;J. Pipher
随着雷神公司2.5微米HgCdTe VIRGO探测器阵列的推出，一些天文计划，如VISTA计划，正在转向雷神公司的近红外探测器阵列。我们表征一个处女座探测器阵列，并提供在低背景下，包括暗电流，读取噪声，总噪声，量子效率和可操作性的测量结果。雷神公司的VIRGO HgCdTe探测器阵列是许多低背景天文计划的优秀候选者，包括星载望远镜任务。
With the introduction of the Raytheon 2.5 micron HgCdTe VIRGO detector array, some astronomy programs, such as the VISTA Program, are turning to Raytheon for near infrared detector arrays. We characterize one VIRGO detector array and provide results of measurements at low backgrounds including dark current, read noise, total noise, quantum efficiency, and operability. The Raytheon VIRGO HgCdTe detector arrays are excellent candidates for many low background astronomical programs, including space-borne telescope missions.