A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2019; you can also visit the original URL.
The file type is application/pdf.
Present State of the Work on Automatic Spectral Classification at Tartu
1984
International Astronomical Union Colloquium
Preserved Fulltext
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.
doi:10.1017/s025292110010675x
fatcat:fq2bx3qxcjggdmanbeakkevnsq