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KASINICS: Near infrared camera system for the BOAO 1.8 m telescope

  • Bongkon Moon
  • , Ho Jin
  • , In Soo Yuk
  • , Sungho Lee
  • , Uk Won Nam
  • , Sang Mok Cha
  • , Seoung Hyun Cho
  • , Jae Mann Kyeong
  • , Youngsik Park
  • , Seungwon Mock
  • , Jeong Yeol Han
  • , Dea Hee Lee
  • , Jang Hyun Park
  • , Wonyong Han
  • , Soojong Pak
  • , Geon Hee Kim
  • , Yong Ha Kim

Research output: Contribution to journalArticlepeer-review

8 Citations (Scopus)

Abstract

We developed Korea Astronomy and Space science Institute (KASI) Near Infrared Camera System (KASINICS) to be installed on the 1.8 m telescope of Bohyunsan Optical Astronomy Observatory (BOAO) in Korea. We use a 512 × 512 InSb array (Aladdin III Quadrant, Raytheon Co.) to enable L band observations as well as J, H, and Ks bands. The field-of-view of the array is 3′.3 × 3′.3 with a resolution of 0″.39/pixel. We adopt an Offner relay optical system, which provides a cold stop to eliminate thermal background emission from the telescope structures. Most parts of the camera, including the mirrors, were manufactured from the same ingot of aluminum alloy to ensure a homologous contraction from room temperature to 80 K. We also developed a readout electronics system for the array detector. Based on preliminary results from test observations, the limiting magnitudes are J = 17.6, H = 17.5, Ks = 16.1, and L(narrow) = 10.0mag at a signal-to-noise ratio of 10 for an integration time of 100s.

Original languageEnglish
Pages (from-to)849-856
Number of pages8
JournalPublication of the Astronomical Society of Japan
Volume60
Issue number4
DOIs
Publication statusPublished - 2008

Keywords

  • Infrared: general
  • Instrumentation: detectors
  • Techniques: Photometric

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