1 June 1994 Astronomical uses of integral field spectrography: present applications at CFHT and future developments
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Abstract
Since the digital detectors (like CCDs) presently available for astronomical instruments have two dimensions only, there is an obvious problem for obtaining detailed spectroscopic information on extended astronomical objects (e.g. active galaxies, regions of star formation, globular clusters, etc.); the classical long- slit spectrographic techniques are grossly inadequate. Several so-called integral field spectrographs (IFS) have been used at the Canada-France-Hawaii telescope during the past years to improve this situation. They typically provide hundreds of spectra in a small (approximately 10' by 10') field with a subarcsecond spatial resolution capability and hundreds of spectral elements, both simultaneously accessed. We describe these various instruments and their present performances, review a few illustrative results obtained with CFH telescope and discuss the expected developments: use of IFS in combination with adaptive optics systems for the study of individual objects at spatial resolution near the 0.1' level, as well as their potential capabilities on Very Large Telescopes, with or without adaptive optics.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christian Vanderriest, Roland Bacon, Yvon Georgelin, Etienne LeCoarer, Guy J. Monnet, "Astronomical uses of integral field spectrography: present applications at CFHT and future developments", Proc. SPIE 2198, Instrumentation in Astronomy VIII, (1 June 1994); doi: 10.1117/12.176823; https://doi.org/10.1117/12.176823
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KEYWORDS
Iterated function systems

Spectrographs

Spectral resolution

Telescopes

Galactic astronomy

Astronomy

Adaptive optics

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