Recent Focal Plane Arrays for Astronomy and Remote Sensing Applications at RVS

被引:1
|
作者
Peralta, Richard J. [1 ]
Beuville, Eric [1 ]
Corrales, Elizabeth [1 ]
Drab, John [1 ]
Erving, Shawn [1 ]
Gin, Andrew [1 ]
Mills, Robert [1 ]
Rabkin, Charles [1 ]
机构
[1] Raytheon Vis Syst, Goleta, CA 93117 USA
来源
HIGH ENERGY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY IV | 2010年 / 7742卷
关键词
FPA; Infrared; Visible; Si PIN; HgCdTe; Si:As; VIRGO; VISTA; Bepi Colombo; VIHI; STC/HRIC; Aquarius;
D O I
10.1117/12.858290
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Raytheon Vision Systems (RVS) arrays are being deployed world-wide in ground based and space based platforms. RVS has a family of high performance visible through far infrared detector arrays for astronomy and civil space applications. Unique and off-the-shelf product lines are readily available to the community. Large sensor chip assemblies using various detector materials like Si PIN, HgCdTe, InSb, and Si: As IBC, covering a detection range from visible (400nm) to mid-wave infrared (28um, MWIR) have been demonstrated with excellent quantum efficiency, dark current, and uniformity. These focal plane arrays have been designed using state-of-the-art low noise, low power, and radiation hardened readout integrated circuits. Complete with optical filters, opto-mechanical packaging, active thermal cooling with matching thermal straps, and optional electronics, RVS provides complete solutions for a multitude of sensor types and mission objectives. This paper describes the recent developments of focal plane assemblies for upcoming missions and telescope platforms.
引用
收藏
页数:12
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