Abstract
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.
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References
Campbell, B.: 1973, Astron. J. 83, pp.1430–1437.
Christensen, C.: 1978, Astron. J. 83, pp. 244–265.
Malyuto, V.: 1977, Tartu Astrofuus. Obs. Publ. 45, pp.150–172.
Malyuto, V., Pelt, J.: 1981, Preprint of the Academy of Sciences of the Estonian SSR, A-1, pp.3–15.
Malyuto, V., Pelt, J.: 1982, CDS Inf. Bull., No. 23, pp.39–40.
Nissen, P.: 1981, Astron. Astrophys. 97, pp.145–175.
West, R.: 1973, in C. Fehrenbach and B.E. Westerlund (eds.), “Spectral Classification and Multicolor Photometry”, IAU Symp. 50, pp.189–124.
Wilson, O.C.: 1976, Astroph. J. 205, 823.
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© 1984 D. Reidei Publishing Company
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Malyuto, V. (1984). Present State of the Work on Automatic Spectral Classification at Tartu. In: Capaccioli, M. (eds) Astronomy with Schmidt-Type Telescopes. Astrophysics and Space Science Library, vol 110. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6387-0_48
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DOI: https://doi.org/10.1007/978-94-009-6387-0_48
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-6389-4
Online ISBN: 978-94-009-6387-0
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