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Title:
Automatic spectral classification
Authors:
Kurtz, M. J.
Affiliation:
AA(Dartmouth Coll., Hanover, NH.)
Publication:
Ph.D. Thesis Dartmouth Coll., Hanover, NH.
Publication Date:
00/1982
Category:
Astronomy
Origin:
STI
NASA/STI Keywords:
CROSS CORRELATION, MULTIVARIATE STATISTICAL ANALYSIS, PATTERN RECOGNITION, CLASSIFICATIONS, DATA REDUCTION, LUMINOSITY, OPEN CLUSTERS, SPECTROPHOTOMETERS, SPECTROSCOPY
Bibliographic Code:
1982PhDT.........2K

Abstract

The use of cross correlation (C.C.), and techniques of Multivariate Analysis and Pattern Recognition in the classification of stellar spectra are presented using an array of spectroscopic standards observed at low (14A) resolution with a digital spectrophotometer. The HR diagram for the faint young open cluster Trumpler 1 was obtained. C.C. is first used to investigate several possible methods of data reduction. The C.C. classification obtained using the optimum reduction techniques obtains a poor luminosity classification, and for nonsupergiants in the spectral range BO-M2 a mean error of 2.2 subtypes. Using Principal Component Analysis it was possible to separate O stars and supergiants earlier than A5 from the rest of the sample, thus resolving a systematic error in the C.C. classification, and achieving a modicum of luminosity discrimination.
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Physics
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