Hostname: page-component-788cddb947-jbkpb Total loading time: 0 Render date: 2024-10-14T13:01:49.706Z Has data issue: false hasContentIssue false
  • English
  • Français

The O.A.O. Spectronebulagraph and the Kyoto 3D Spectrograph

Published online by Cambridge University Press:  12 April 2016

Hiroshi Ohtani
Hiroshi Ohtani*
Affiliation:
Department of Astronomy, Kyoto University Kyoto 606-01, Japan

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.

Spectronebulagraph, an automated observation system of tridimensional spectroscopy with a long slit spectrograph, is now in operation at the 188 cm telescope of the Okayama Astrophysical Observatory. This system is based on the local area net work of personal computers which control the telescope, the autoguider, the Cassegrain spectrograph and its CCD camera. Effects of variable atmospheric transmission during scans of target objects are removed by performing a set of two orthogonal scans and the data processing.

A new spectrograph is now under development for the telescope. This instrument has multiple modes for tridimensional spectroscopy, i.e., the filter imagery mode, the imaging Fabry-Perot interferometer mode, a slit spectrograph mode for Spectronebulagraph, and the microlens array spectrograph (TIGER) mode. For the last mode, a dual preoptics to get simultaneously the sky background is introduced and achromatization of the microlenses is tried. This project is a part of development of a prototype instrument for the SUBARU telescope.

Type
3. Integral Field Spectrographs and Spectrometers
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 195 - 202
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Clark, D. and Wallace, P., 1984, QJRAS, 25, 114.Google Scholar
Courtes, G., Georgelin, Y., Bacon, R., Monnet, G. and Boulesteix, J., 1988, inInstrumentation for ground based optical astronomy, ed. Robinson, L.B., Springer-Verlag, New York, p 267.Google Scholar
Kosugi, G., Ohtani, H., Yoshida, M., Sasaki, T., Shimizu, Y., Koyano, H., Aoki, K., Sasaki, M., 1994, to be submitted to PASP.Google Scholar
Ohtani, H., Sasaki, M., Aoki, K., Takano, E., Kiyohara, M., 1994, in the Proceedings of Instrumentation in Astronomy VIII, in press.Google Scholar