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Automatic Classification of Objective Prism Spectra
Published online by Cambridge University Press: 14 August 2015
Abstract
Methodological problems and hardware/software requirements of efficient automatic classification of objective prism stellar spectra are described on the basis of experience from ‘microphotometer-computer’ classification. Significant advances in hardware (two-dimensional scanners, on-line computers) as well as in software (image processing techniques) have now brought high-speed, exhaustive, automatic classification within reach. Some astronomical implications of automatic spectral surveys are discussed.
- Type
- Part II: Classification of Objective-Prism Spectra
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- Copyright
- Copyright © Reidel 1973
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