Paper
19 July 2010 Repackaging and characterizing of a HgCdTe CMOS infrared camera for the New Solar Telescope
Wenda Cao, Roy Coulter, Nicolas Gorceix, Philip R. Goode
Author Affiliations +
Abstract
The 1.6-meter New Solar Telescope (NST) is currently the world's largest aperture solar telescope. The NST is newly built at Big Bear Solar Observatory (BBSO). Among other instruments, the NST is equipped with several focal plane instruments operating in the near infrared (NIR). In order to satisfy the diverse observational requirements of these scientific instruments, a 1024 × 1024 HgCdTe TCM8600 CMOS camera manufactured by Rockwell Scientific Company has been repackaged and upgraded at Infrared Laboratories Inc. A new ND-5 dewar was designed to house the TCM8600 array with a low background filter wheel, inverted operation and at least 12 hours of hold time between fills. The repackaged camera will be used for high-resolution NIR photometry at the NST Nasmyth focus on the telescope and high-precision NIR spectro-polarimetry in the NST Coud´e Lab below. In March 2010, this repackaged camera was characterized in the Coud´e Lab at BBSO. This paper presents the design of new dewar, the detailed process of repackaging and characterizing the camera, and a series of test results.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Wenda Cao, Roy Coulter, Nicolas Gorceix, and Philip R. Goode "Repackaging and characterizing of a HgCdTe CMOS infrared camera for the New Solar Telescope", Proc. SPIE 7742, High Energy, Optical, and Infrared Detectors for Astronomy IV, 774220 (19 July 2010); https://doi.org/10.1117/12.856616
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Cited by 4 scholarly publications.
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KEYWORDS
Cameras

Staring arrays

Infrared cameras

Optical filters

Infrared imaging

Solar telescopes

Infrared radiation

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