Paper
10 July 2008 GHαFaS: galaxy Hα Fabry-Perot system for the WHT
Claude Carignan, Olivier Hernandez, Jean-Luc Gach, Philippe Balard, Marie-Maude De Denus-Baillargeon, Kambiz Fathi, John Beckman, Jean Koulidiati
Author Affiliations +
Abstract
GHαFaS is a new Fabry-Perot system available at the William Herschel Telescope. It was mounted, for the first time, at the Nasmyth focus of the 4.2 m WHT in La Palma in 2007 July. With a spectral resolution of the order R~15000 and a seeing limited spatial resolution, GHαFaS provides a new look at the Hα-emitting gas over a 4 arcminutes circular field in the nearby universe. Many types of objects can be observed with a scanning Fabry-Perot system on a 4.2 m class telescope such as galaxies, HII regions, planetary nebulae, supernova remnants outflows from stars and the diffuse interstellar medium. Astronomers from the Laboratoire d'Astrophysique Experimentale (LAE) in Montreal, the Laboratoire d'Astrophysique de Marseille (LAM), and the Instituto de Astrofisica de Canarias (IAC), have inaugurated GHαFaS by studying in detail the dynamics of nearby spiral galaxies. A robust set of tools for reducing and analyzing the data cubes obtained with GHαFaS has also been developed.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Claude Carignan, Olivier Hernandez, Jean-Luc Gach, Philippe Balard, Marie-Maude De Denus-Baillargeon, Kambiz Fathi, John Beckman, and Jean Koulidiati "GHαFaS: galaxy Hα Fabry-Perot system for the WHT", Proc. SPIE 7014, Ground-based and Airborne Instrumentation for Astronomy II, 70145N (10 July 2008); https://doi.org/10.1117/12.790616
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KEYWORDS
Fabry–Perot interferometers

Galactic astronomy

Charge-coupled devices

Signal to noise ratio

Telescopes

Sensors

Calibration

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