CONSTRUCTION OF THE BOAO ECHELLE SPECTROGRAPH (BOES)

보현산천문대 고분산 에셀분광기(BOES) 제작

  • KIM KANG-MIN (Bohyunsan Optical Astronomy Observatory, Korea Astronomy Observatory, Dept. of Astronomy and Atmospheric Sciences, Kyungpook National University) ;
  • JANG JEONG GYUN (Bohyunsan Optical Astronomy Observatory, Korea Astronomy Observatory) ;
  • CHUN MOO-YOUNG (Bohyunsan Optical Astronomy Observatory, Korea Astronomy Observatory) ;
  • PARK BYEONG-GON (Bohyunsan Optical Astronomy Observatory, Korea Astronomy Observatory, Dept. of Astronomy and Atmospheric Sciences, Kyungpook National University) ;
  • HYUNG SIEK (Bohyunsan Optical Astronomy Observatory, Korea Astronomy Observatory) ;
  • HAN INWOO (Bohyunsan Optical Astronomy Observatory, Korea Astronomy Observatory) ;
  • YOON TAE SEOG (Dept. of Astronomy and Atmospheric Sciences, Kyungpook National University) ;
  • VOGT STEVEN S. (Lick Observatory)
  • 김강민 (한국천문연구원 보현산천문대, 경북대학교 천문대기과학과) ;
  • 장정균 (한국천문연구원 보현산천문대) ;
  • 천무영 (한국천문연구원 보현산천문대) ;
  • 박병곤 (한국천문연구원 보현산천문대, 경북대학교 천문대기과학과) ;
  • 형식 (한국천문연구원 보현산천문대) ;
  • 한인우 (한국천문연구원 보현산천문대) ;
  • 윤태석 (경북대학교 천문대기과학과) ;
  • Published : 2000.08.01

Abstract

The BOES (BOAO Echelle Spectrograph), a fiber-fed echelle spectrograph of the BOAO 1.8 m telescope, has been designed and now is being manufactured. The BOES follows a white pupil design collimated with two off-axis parabolic mirrors. The 136mm collimating beam leaving the 41.59 grooves/mm R4 echelle grating is refocused near the narrow folding mirror. Through the two cross-disperser prisms and $\phi250 mm(f/1.5)$ transmission camera, the beam images on EEV $2k\times4k$ CCD. The BOES can take the wavelength range of 3700 to $10100{\AA}$ at a single spot with spectral resolution R = 20000 to 40000 depending on the fiber set employed. We describe the key sciences and performance, current status of construction, and future plan of the BOES.

Keywords