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Development of the Far-ultraviolet Imaging Spectrograph on KAISTSAT-4

Published online by Cambridge University Press:  12 April 2016

Wonyong Han
Affiliation:
Korea Astronomy Observatory, 61-1 Whaam, Yusong, Taejon, 305-348, Korea
Kyoung Wook Min
Affiliation:
Korea Advanced Institute of Science and Technology, 373-1 Kusong, Yusong, Taejon, 305-701, Korea
Jerry Edelstein
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, USA
Uk-Won Nam
Affiliation:
Korea Astronomy Observatory, 61-1 Whaam, Yusong, Taejon, 305-348, Korea
Jong-Ho Seon
Affiliation:
Korea Advanced Institute of Science and Technology, 373-1 Kusong, Yusong, Taejon, 305-701, Korea
Kwang-Il Seon
Affiliation:
Korea Astronomy Observatory, 61-1 Whaam, Yusong, Taejon, 305-348, Korea
Jang-Hyun Park
Affiliation:
Korea Astronomy Observatory, 61-1 Whaam, Yusong, Taejon, 305-348, Korea
In-Soo Yuk
Affiliation:
Korea Astronomy Observatory, 61-1 Whaam, Yusong, Taejon, 305-348, Korea
Ho Jin
Affiliation:
Korea Astronomy Observatory, 61-1 Whaam, Yusong, Taejon, 305-348, Korea
Woo-Baik Lee
Affiliation:
Korea Astronomy Observatory, 61-1 Whaam, Yusong, Taejon, 305-348, Korea
Kyungin Kang
Affiliation:
Korea Advanced Institute of Science and Technology, 373-1 Kusong, Yusong, Taejon, 305-701, Korea
Kwangsun Ryu
Affiliation:
Korea Advanced Institute of Science and Technology, 373-1 Kusong, Yusong, Taejon, 305-701, Korea
Jin-Geun Rhee
Affiliation:
Korea Advanced Institute of Science and Technology, 373-1 Kusong, Yusong, Taejon, 305-701, Korea
Dae-Hee Lee
Affiliation:
Korea Advanced Institute of Science and Technology, 373-1 Kusong, Yusong, Taejon, 305-701, Korea
Eric Korpela
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, USA
W. Van Dyke Dixon
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, USA

Abstract

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The Far-ultraviolet IMaging Spectrograph (FIMS) is a small spectrograph optimized for the observations of diffuse hot interstellar medium in far-ultraviolet wavebands (900–1150Å and 1335–1750Å). The instrument is expected to be sensitive to emission line fluxes an order of magnitude fainter than any previous missions. FIMS is currently under development and is scheduled for launch in 2002.

Type
III. New Trends in Small-Telescope Technology
Copyright
Copyright © Astronomical Society of the Pacific 2001

References

Bowyer, S., Edelstein, J., & Lampton, M. 1998, ApJ, 485, 523 Google Scholar