• The Bulletin of The Korean Astronomical Society
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• v.33 no.1
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• pp.59.2-59.2
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• 2008

• Bulletin of the Korean Space Science Society
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• 1999.09a
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• pp.66-66
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• 1999

No Abstract, See Full Text

• The Bulletin of The Korean Astronomical Society
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• v.27 no.2
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• pp.65-65
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• 2002

• The Bulletin of The Korean Astronomical Society
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• v.32 no.1
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• pp.70.2-70.2
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• 2007

• The Bulletin of The Korean Astronomical Society
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• v.31 no.2
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• pp.70.2-70.2
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• 2006

• The Bulletin of The Korean Astronomical Society
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• v.34 no.1
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• pp.73.1-73.1
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• 2009

• The Bulletin of The Korean Astronomical Society
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• v.34 no.1
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• pp.53.1-53.1
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• 2009

• Bulletin of the Korean Space Science Society
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• 2009.04a
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• pp.58.2-58.2
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• 2009

• Bulletin of the Korean Space Science Society
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• 2009.04a
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• pp.30.4-31
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• 2009

• Journal of The Korean Astronomical Society
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• v.38 no.2
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• pp.69-72
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• 2005

The FIMS (Far-ultraviolet IMaging Spectrograph; also known as SPEAR, Spectroscopy of Plasma Evolution from Astrophysical Radiation) is the primary payload of the STSAT-1, the first Korean science satellite, which was launched in September, 2003. The FIMS performs spectral imaging of diffuse far-ultraviolet emission with the unprecedented wide field of view and the relatively good spectral resolution. We present far-ultraviolet spectral observations of highly ionized interstellar medium including supernova remnants, superbubbles, soft X-ray shadows, and the molecular hydrogen fluorescent emission lines. The FIMS has detected He II, C III, 0 III, O IV, Si IV, O VI, and $H_2$ fluorescent emission lines. The emission lines arise in shocked or thermally heated and in photo-ionized gases. We present an overview of the FIMS instrument and its initial observational results.