9 July 1998 IMACS: the multiobject spectrograph and imager for the Magellan I telescope
Author Affiliations +
The Inamori Magellan Areal Camera and Spectrograph (IMACS) will be one of three first-generation instruments for the Magellan 6.5 m telescopes. It will be installed at the f/11 (Gregorian) Nasmyth focus. This instrument drove the specification and design of the f/11 configuration, which it uses to feed an all-spherical, wide-field collimator. The combination of the Gregorian secondary and refracting collimator lead to 0.2 arc-sec images over a 17 arc-min field with an f/2.66 camera, and 0.4 arc-sec images over a 27 arc- min field with an f/1.49 camera. This paper describes the preliminary specifications for the multiple spectrographic and imaging modes, the optical layout of the instrument and Epps cameras, and strategies for the design and fabrication of the instrument.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bruce C. Bigelow, Alan M. Dressler, Stephen A. Shectman, and Harland W. Epps "IMACS: the multiobject spectrograph and imager for the Magellan I telescope", Proc. SPIE 3355, Optical Astronomical Instrumentation, (9 July 1998); doi: 10.1117/12.316760; https://doi.org/10.1117/12.316760


The LAMOST middle resolution spectrograph
Proceedings of SPIE (July 05 2018)
Las Campanas Observatory
Proceedings of SPIE (July 09 2018)
Wide-field fast scanning spectrograph
Proceedings of SPIE (August 26 2003)

Back to Top