  In this paper, we present a catalogue of the spectra of bright stars observed
during the sky survey using the Far-Ultraviolet Imaging Spectrograph (FIMS),
which was designed primarily to observe diffuse emissions. By carefully
eliminating the contamination from the diffuse background, we obtain the
spectra of 70 bright stars observed for the first time with a spectral
resolution of 2--3 {\AA} over the wavelength of 1370--1710 {\AA}. The
far-ultraviolet spectra of an additional 139 stars are also extracted with a
better spectral resolution and/or higher reliability than those of the previous
observations. The stellar spectral type of the stars presented in the catalogue
spans from O9 to A3. The method of spectral extraction of the bright stars is
validated by comparing the spectra of 323 stars with those of the International
Ultraviolet Explorer (IUE) observations.
