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2001•International Astronomical Union ColloquiumOpen access

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

Wonyong Han, K. W. Min, Jerry Edelstein, Uk‐Won Nam, Jongho Seon, Kwang‐Il Seon, Jang‐Hyun Park, In-Soo Yuk, Ho Jin, Woo‐Baik Lee, Kyung-In Kang, Kwangsun Ryu, Jin-Geun Rhee, Daehee Lee, Eric Korpela, W. V. Dixon

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Abstract

Abstract 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.

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Abstract 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.

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Available abstract

Abstract 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.

Key concepts: Spectrograph, Ultraviolet, Far ultraviolet, Physics, Extreme ultraviolet, Optics, Astronomy, Spectral line

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