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Multifiber Spectroscopy for the Keck 10-Meter Telescope

Oke, J. B. (1988) Multifiber Spectroscopy for the Keck 10-Meter Telescope. In: Instrumentation for Ground-Based Optical Astronomy: Present and Future. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer , New York, NY, pp. 256-259. ISBN 978-1-4612-8387-4. http://resolver.caltech.edu/CaltechAUTHORS:20190610-102638936

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Abstract

Present day spectrographs with their excellent coatings and high quantum efficiency CCDs have reached levels of performance which cannot easily be exceeded by significant factors. To achieve still higher efficiency it is necessary to observe many objects simultaneously either with slit-mask or multi-fiber techniques. It is therefore planned to implement both techniques on the Keck 10-meter telescope. Multi-slit or slit-mask devices will be implemented on both the low-resolution and moderate-resolution instruments. Because of the limited space at the Cassegrain focus the multi-fiber mode will be implemented only on the Moderate Resolution Imaging Spectrometer (MRIS) and the high resolution instrument which are located on the Nasmyth platform. In this talk I will briefly describe the MRIS and indicate how we plan to implement the fiber mode.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-1-4612-3880-5_24DOIArticle
Additional Information:© 1988 Springer-Verlag New York Inc.
Subject Keywords:Faint Object; Fiber Feed; High Resolution Instrument; Fiber Head; Moderate Resolution Image Spectrometer
Record Number:CaltechAUTHORS:20190610-102638936
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190610-102638936
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96237
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:10 Jun 2019 17:31
Last Modified:10 Jun 2019 17:31

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