Determination of Atmospheric Extinction Coefficient at Bohyunsan Optical Astronomy Observatory

Details Determination of Atmospheric Extinction Coefficient at Bohyunsan Optical Astronomy Observatory Determination of Atmospheric Extinction Coefficient at Bohyunsan Optical Astronomy Observatory

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pkas...12..167k&link_type=abstract

Publications of the Korean Astronomical Society, vol.12, no.1, p.167-172

Astronomy and Astrophysics

Astronomy

Scientific paper

Detailed low spectral resolution observations of the spectrum have been made for three early spectral type standard stars, HR718, HR1544, HR3454, respectively, for the wavelength region 4,300A to 7,500A, using the Bohyunsan Optical Astronomy Observatory(BOAO) Middle-Dispersion Spectrograph. These standard stars were chosen from well-known bright northern standard stars. All of the observed long slit spectral data has been reduced and analyzed using the IRAF reduction procedure. The derived extinction coefficients are compared with the other observatory result. The derived value can be used in the determination of flux calibration of BOAO spectroscopic observation. However, until the high quality data are secured from a new series of observation in the blue region and are re-analyzed, together, the extinction coefficients below the 4,000A wavelength remains unknown.

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