Abstract
Spectrographs using plane aspherized gratings have excellent resolution over a wide field and require one less element than a conventional Schmidt or Maksutov camera. However, they are restricted to configurations where the grating is approximately normal to the camera axis.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Richardson, E.H., Brealey, G.A. and Dancey, R. 1971, Publ. Dom. astrophys. Obs. 14, p. 1 (also Proc. ESO/CERN Conference 1972, ed. S. Laustsen and A. Reiz, pp. 275–284).
Richardson, E.H. 1975, “CFHT: Optical Design of 10cm and 30cm Grating Spectrographs”, CFHT Corporation, Hawaii, April 1975.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1982 D. Reidel Publishing Company
About this paper
Cite this paper
Richardson, E.H. (1982). Optical Designs of Plane Aspherized Grating Spectrographs. In: Humphries, C.M. (eds) Instrumentation for Astronomy with Large Optical Telescopes. Astrophysics and Space Science Library, vol 92. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7787-7_17
Download citation
DOI: https://doi.org/10.1007/978-94-009-7787-7_17
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-7789-1
Online ISBN: 978-94-009-7787-7
eBook Packages: Springer Book Archive