Hostname: page-component-5c6d5d7d68-7tdvq Total loading time: 0 Render date: 2024-08-20T13:51:38.606Z Has data issue: false hasContentIssue false

Slitless Spectroscopy of Stars with Grating-Prism and Focal Reducer Techniques

Published online by Cambridge University Press:  12 April 2016

E. H. Geyer*
Affiliation:
Sternwarte der Universität Bonn

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.

A slitless field spectrograph for Cassegrain telescopes has been designed. It is based on the focal reducer optical arrangement and grating prisms. Together with the “multiple diaphragm method” not only a gain in limiting magnitude of 3 to 4 magnitudes has been achieved, but also other drawbacks of the classical objective prism camera are avoided.

Type
V Classification related Spectrophotometry by Classical Techniques and by New Registration and Detection Methods
Copyright
Copyright © Vatican Observatory 1979

References

Courtes, G. (1960). Ann d’Astrophys. 23, 115.Google Scholar
Fehrenbach, Ch. (1947). Ann d’Astrophys. 10, 306.Google Scholar
Fraunhofer, J. V. (1817). Denkschriften Akad. d. Wiss. München 5, 193.Google Scholar
Geyer, E. H. (1966). Veröff, . Landessternwarte Heidelberg-Königtistuhl 18, 1.Google Scholar
Geyer, E. H. (1972). Proceedings of ESO-SRC conference on “The Role of Schmidt Telescopes in Astronomy”, p. 61.Google Scholar
Geyer, E. H. and Schmidt, H. (1976). Mitt. Astron. Gesellsch. 40, 125.Google Scholar
Hellerich, J. (1938). Mitt. Hamburger Steérnwarte No. 43, 179.Google Scholar
Meinel, A.B. (1956). Astrophys. J. 124, 652.Google Scholar
Nelles, B. (1978). Diplomarbeit Physik, Universität Bonn.Google Scholar
Secchi, A. (1878). Die Sterne - Grundzuge der Astronomie der Fixsterne, p. 78; F. A. Brockhaus Verlag, Leipzig.Google Scholar