[An automated stellar spectra classification system based on non-parameter regression and nearest neighbor method].
The automated classification and recognition of stellar spectra is an important research for the spectra processing system of modem telescope survey project. For the spectra without flux calibration, the authors present an automated stellar spectra classification system to achieve two goals: one is the spectral class and spectral subclass classification, and the other is luminosity type recognition. The system is composed of three units: (1) continuum normalization method based on wavelet technique; (2) non-parameter regression method for spectral class and spectral subclass classification; (3) chi2 method based on nearest neighbor for luminosity type determination. The experiments on low-resolution spectra show that the system achieves 3.2 spectral subclass precision for spectral and spectral subclass classification, 60% correct rate for luminosity recognition, and 78% rate for the luminosity recognition with error less than or equal to 1. The system is easy, rapid in training, and feasible for the automated spectra classification.
Zhang
Jian-Nan
JN
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China. jnzhang@lamost.org
Zhao
Yong-Heng
YH
Liu
Rong
R