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Volumn 35, Issue 1, 2007, Pages 157-160
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A method for auto-recognizing the M-type stars based on wavelet feature
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Author keywords
Astronomical spectra; Characteristic frequency; Detection of absorption bands; Wavelet feature; Wavelet transform
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Indexed keywords
ABSORPTION SPECTRA;
ASTRONOMY;
MATHEMATICAL TRANSFORMATIONS;
WAVELENGTH;
WAVELET TRANSFORMS;
ABSORPTION BANDS DETECTION;
ASTRONOMICAL SPECTRA;
CELESTIAL BODY;
CHARACTERISTIC FREQUENCY;
CORRECT RATE;
LAMOST PROJECT;
M TYPE STARS;
SKY SURVEY PROJECT;
STAR EVOLUTION;
WAVELENGTH REGION;
WAVELET FEATURE;
STARS;
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EID: 34147206696
PISSN: 03722112
EISSN: None
Source Type: Journal
DOI: None Document Type: Article |
Times cited : (13)
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References (9)
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