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Fabry-Perot Spectrographs for VLT's

Published online by Cambridge University Press:  12 April 2016

Guy Monnet
Guy Monnet*
Affiliation:
Observatoire de Lyon, F-69230 Saint Genis Laval

Extract

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Four Reasons are advocated to stress the interest of Fabry-Perot Spec-trographs (F.P.S.) as potentially useful instruments for the future Very Large Telescopes :

  1. - Reasonably wide spectrum of Astronomical uses

  2. - Good use of Telescope area

  3. - Relative cheapness

  4. - Versatility

Type
IV. Instrumentation - Components
Information
International Astronomical Union Colloquium , Volume 79: Very Large Telescopes, their Instrumentation and Programs , 1984 , pp. 493 - 496
Copyright
Copyright © ESO 1984

References

Bouleateix, J., Georgelin, Y., Marcelin, M. and Fort, J., 1981, IAU Colloquium n° 67, Zelenchuk, Ed. Reidel, , p. 223.Google Scholar
Buisson, H., Fabry, Ch. and Bourget, H., 1914, Astrophys. J. 40, 241.Google Scholar
Carranza, G., Courtés, G., Georgelin, Y., Monnet, G., Pourcelot, A. and Astier, N., 1968, Ann. Astrophys. 31, 63.Google Scholar
Roesler, F., Oliversen, R., Scherb, F., Lattis, J., Williams, T., York, D., Jenkins, E., Lowrance, J., Zucchine, P., and Long, D., 1982, Astrophys. J. 259, 900.Google Scholar
Taylor, K. and Atherton, P., 1980, Mon. Not. R. astr. Soc. 191, 675.Google Scholar
Tully, R., 1974, Astrophys. J. Suppl. Ser. n° 251, 27, 415.CrossRefGoogle Scholar
Vaucouleurs, G. and A. de, and Pence, W., 1974, Astrophys. J. Lett. 194, L 119.Google Scholar