IGRINS : Collimating Mirror Mount Opto-mechanical Design

  • Rukdee, Surangkhana (University of Science and Technology) ;
  • Park, Chan (Korea Astronomy and Space Science Institute) ;
  • Chun, Moo-Young (Korea Astronomy and Space Science Institute) ;
  • Yuk, In-Soo (Korea Astronomy and Space Science Institute) ;
  • Lee, Sung-Ho (Korea Astronomy and Space Science Institute) ;
  • Lee, Han-Shin (University of Texas at Austin) ;
  • Kim, Kang-Min (Korea Astronomy and Space Science Institute) ;
  • Jeong, Hwa-Kyung (Korea Astronomy and Space Science Institute) ;
  • Strubhar, Joseph (University of Texas at Austin) ;
  • Jaffe, Daniel T. (University of Texas at Austin)
  • Published : 2011.04.15

Abstract

The Korea Astronomy and Space Science Institute (KASI) and the Department of Astronomy at the University of Texas at Austin (UT) are developing a near infrared wide-band high resolution spectrograph, IGRINS (Immersion Grating Infrared Spectrograph). The white-pupil design of the instrument optics uses 7 cryogenic mirrors including 3 aspherical off-axis collimators and 4 flat fold mirrors. Two of the 3 collimators are H- and K-band pupil transfer mirrors and they are designed as compensators for the system alignment in each channel. Therefore, their mount design will be one of the most sensitive parts in the IGRINS optomechanical system. The design work will include the computer-aided 3D modeling and finite element analysis (FEA) to optimize the structural stability of the mount models. The mount body will also include a tip-tilt and translation adjustment mechanism to be used as the alignment compensators.

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