English

CIRPASS: description, performance and astronomical results

Astrophysics 2009-11-10 v1

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.

Keywords

Cite

@article{arxiv.astro-ph/0408189,
  title  = {CIRPASS: description, performance and astronomical results},
  author = {Ian Parry and Andrew Bunker and Andrew Dean and Michelle Doherty and Anthony Horton and David King and Marie Lemoine-Busserole and Craig Mackay and Richard McMahon and Steve Medlen and Rob Sharp and Joanna Smith},
  journal= {arXiv preprint arXiv:astro-ph/0408189},
  year   = {2009}
}

Comments

SPIE conference procedings, 5492-50, 10 pages

R2 v1 2026-07-22T08:41:14.740Z