Bright stars observed by FIMS/SPEAR

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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 angstrom over the wavelength o1370- 1710 angstrom. 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
Publisher
OXFORD UNIV PRESS
Issue Date
2016-02
Language
English
Article Type
Article
Keywords

HOPKINS-ULTRAVIOLET-TELESCOPE; SKY-SURVEY TELESCOPE; SPECTRAL CLASSIFICATION; STELLAR SPECTRA; OB STARS; CALIBRATION; PERFORMANCE; SATELLITE; SPECTROGRAPH; PARAMETERS

Citation

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v.456, no.1, pp.417 - 430

ISSN
0035-8711
DOI
10.1093/mnras/stv2670
URI
http://hdl.handle.net/10203/207655
Appears in Collection
PH-Journal Papers(저널논문)
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