arXiv · astro-ph/0408189
CIRPASS: description, performance and astronomical results
Abstract
The Cambridge Infra-red Panoramic Survey Spectrograph (CIRPASS) is described. This near-infrared (NIR) spectrograph has been used on the 8m Gemini-South Telescope, the 3.9m Anglo-Australian Telescope (AAT) and the 4.2m William Herschel Telescope (WHT). Its performance in both integral field mode and multi-object mode is discussed and some scientific highlights are presented. A multi-IFU system, which is currently under construction, is also described.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Ian Parry, Andrew Bunker, Andrew Dean, Michelle Doherty, Anthony Horton, David King, Marie Lemoine-Busserole, Craig Mackay, Richard McMahon, Steve Medlen, Rob Sharp, Joanna Smith. 2004-08-10. CIRPASS: description, performance and astronomical results. https://doi.org/10.1117/12.552012
Cite the original work for its findings. Save a collection to share your selection of sources.