Hostname: page-component-84b7d79bbc-7nlkj Total loading time: 0 Render date: 2024-07-27T20:23:07.439Z Has data issue: false hasContentIssue false

ESO 16 Metre Very Large Telescope - Instrument Matching in Spectroscopy and Direct Imaging

Published online by Cambridge University Press:  12 April 2016

Daniel Enard*
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-8046 Garching bei München, FRG

Extract

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.

Preliminary feasibility studies have been carried out in the framework of the ESO VLT project which have permitted the evaluation of several possible approaches to the instrument matching problem. This paper briefly discusses the detector long term perspective, recalls the main scaling laws and attempt to provide some quantitative analysis of spatial performance of instrumentation in a few typical cases. Field slicing technique is proposed as a potential solution to solve detector matching problems.

Type
IV. Instrumentation - Components
Copyright
Copyright © ESO 1984

References

1) Cullum, M., Optical detectors and the VLT. ESO Workshop on ESO’s VLT, Cargèse May 1983.Google Scholar
2) Hilvak, P.J., Henry, P.J., Pilcher, C.B., Proceedings of Instrumentation in Astronomy, London Sept.1983, SPIE Vol. 446 Google Scholar
3) Wright, J.F., Mackay, C.D., Proceedings SPIE 290, p. 160.Google Scholar
4) Goldman, S., Information theory, Dover Publ. New-York.Google Scholar
5) Faber, S.M., UC. TMT report. AV 61.Google Scholar
6) Richardson, H., Prime focus corrector lens for a 300” telescope.Google Scholar
7) Delabre, B., ESO internal communication.Google Scholar
8) Buzzoni, B., Enard, D., Ferlet, R., Lund, G., to be published in “The Messenger”.Google Scholar