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CIRPASS

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Date

2004

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Abstract

The Cambridge Infra-red Panoramic Survey Spectrograph (CIRPASS) is described. This near-infrared (MR) 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.

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Citation

URI

https://dspace-test.anu.edu.au/handle/1885/733742794

Collections

DevOps Pure Testing

Source

Proceedings of SPIE - The International Society for Optical Engineering

Type

Conference article

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DOI

10.1117/12.552012

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