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Present State of the Work on Automatic Spectral Classification at Tartu

Published online by Cambridge University Press:  12 April 2016

V. Malyuto
V. Malyuto*
Affiliation:
W. Struve Tartu Astrophysical Observatory, Toravere, Estonia, USSR

Extract

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An automatic spectral classification technique for objective-prism spectra is being developed.The procedure of selecting standard stars is described.The applicability of a linear polynomial regression model for choosing and calibrating the spectral criteria for Teff, Mv, [Fe/H] is demonstrated.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 78: Astronomy with Schmidt-type telescopes , 1984 , pp. 287 - 290
Copyright
Copyright © Reidel 1984

References

Campbell, B.: 1979, Astron. J. 33, pp.1430–1437.Google Scholar
Christensen, C: 1973, Astron. J. 83, pp.244–205.CrossRefGoogle Scholar
Malyuto, V.: 1977, Tartu Astrofuus. Obs. Publ. 45, pp. 158-172.Google Scholar
Malyuto, V., Pelt, J.: 1981, Preprint of the Academy of Sciences of the Estonian SSR, A-l, pp.3–15.Google Scholar
Malyuto, V., Pelt, J.: 1982, CDS Inf. Bull., No.23, pp.39–40.Google Scholar
Nissen, P.: 1981, Astron. Astrophys. 97, pp.145–175.Google Scholar
West, R.: 1973, in Fehrenbach, C. and Westerlund, B.E. (eds.), “Spectral Classification and Multicolor Photometry”, IAU Symp. 50, pp.109–124.Google Scholar
Wilson, O.C.: 1970, Astroph. J. 205, 823.CrossRefGoogle Scholar