Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-24T16:37:41.032Z Has data issue: false hasContentIssue false
  • English
  • Français

Un Spectrographe a Reseau Aspherique pour Telescope f/4*

Published online by Cambridge University Press:  12 April 2016

G. Lemaître
G. Lemaître*
Affiliation:
Observatoire de Marseille, 2 Place Le Verrier, F-13248 Marseille Cedex 4, 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.

Aspheric diffraction gratings have been produced by the elastic relaxation method. These gratings lead to more efficient spectrograph mounting arrangements since, for a wide field instrument of fast aperture ratio, a smaller number of optical surfaces are required. The UV-PRIM spectrograph is the first instrument of this type to have been constructed.

Type
Section II: Spectrographs and Spectrometers
Information
International Astronomical Union Colloquium , Volume 67: Instrumentation for Astronomy with Large Optical Telescopes , 1982 , pp. 137 - 141
Copyright
Copyright © Reidel 1982

Footnotes

*

Communication présentée par G. Wlérick

References

Lamaître, G.: Janvier 1974, Thèse, Université de Provence, Aix-Marseilie I.Google Scholar
Lemaître, G.: 1977, Astron. Astrophys. 59, 249.Google Scholar