Hostname: page-component-76fb5796d-dfsvx Total loading time: 0 Render date: 2024-04-26T06:30:27.256Z Has data issue: false hasContentIssue false
  • English
  • Français

3D Spectroscopy with large Telescopes: past, present and prospects

Published online by Cambridge University Press:  12 April 2016

G. Monnet
G. Monnet*
Affiliation:
Observatoire de Lyon, 69561 Saint-Genis-Laval Cedex, France

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The dimensional curse of having to pack 3D spectrophotometry data on solely 2D detectors is briefly discussed, and the main astronomical domains covered by 3D spectroscopy introduced. Finally, the scientific case for high spatial resolution 3D techniques coupled to Adaptive Optics capabilities is presented, with special emphasis on the observation of the nuclei of galaxies.

Type
1. Basic Principles, Focal Reducers
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 12 - 17
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Bacon, R., Emsellem, E., Monnet, G., Nieto, J.L. 1994, A&A, 281, 691 Google Scholar
Boulesteix, J., Georgelin, Y., Marcelin, M., Monnet, G., in S.P.I.E. Conf. Inst. Astr.: 1983, vol. V, 445 Google Scholar
Buisson, H., Fabry, Ch., Bourget, H. 1914, ApJ, 40, 241 Google Scholar
Carranza, G., Courtès, G., Georgelin, Y., Monnet, G., Pourcelot, A. 1968, Ann. d’Ap., 31, 63 Google Scholar
Courtès, G. 1972, Vistas in Astron., 14, 163 Google Scholar
Taylor, K., Atherton, P. 1980, MNRAS, 191, 675 Google Scholar
Tully, R.B. 1974, ApJS, 27, 415 Google Scholar
Vanderriest, C., Courtès, G., Donas, J. 1984, J. Optics (Paris), 15, n° 4 bis, 237 Google Scholar
Wilkinson, A., Sharpies, R.H., Fosbury, R.A.E., Wallace, P.T. 1986, MNRAS, 218, 297 Google Scholar