Final integration of the Gemini High-Resolution Optical SpecTrograph (GHOST) spectrograph
作者
John Pazder,Alan W. McConnachie,Michael Ireland,André Anthony,John Bassett,Greg Burley,Edward L. Chapin,Vladimir Churilov,A. Densmore,Jennifer Dunn,Tony Farrell,David K. Henderson,Brian Hoff,Jordan Lothrop,Scott MacDonald,S. Margheim,В. А. Решетов,Ivan Wevers,Lewis Waller,P. Young
标识
DOI:10.1117/12.2630715
摘要
The Gemini High-Resolution Optical SpecTrograph (GHOST) instrument is the next generation high resolution spectrograph for the Gemini telescope. The GHOST instrument was developed for the Gemini telescope as a collaboration between Australian Astronomical Optics (AAO) at Macquarie University, the Herzberg Astronomy and Astrophysics (HAA) in Canada and the Australian National University (ANU). The instrument is a fiber fed spectrograph with R<50,000 in two-object mode and R<75,000 in single object mode. The bench spectrograph was integrated at Gemini South from April to June 2022. This paper presents the final integration and alignment of the spectrograph at Gemini South and the measured spectrograph performance at the telescope.