The Application of Artificial Neural Networks: A Catalog of Spectral Indices

Computer Science – Databases

Scientific paper

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Scientific paper

With the improvements in observational tools, it is feasible to have a larger databases of low resolution spectroscopy. In order to extract observational and physical properties from such databases, it is necessary to employ computer methods, such as artificial neural networks and principal component analysis. Our group is involved in investigating the potential of new tools to derive stellar classification and atmospheric parameters from low resolution spectroscopy (see e.g. Gulati et al., 1994, 426, 340; Gulati et al., 1997, 322, 933; Singh et al., 1998, MNRAS, 295, 312). I would like to present the current status of automating this process. We envisage the use of such methods for study of the stellar content of stellar systems whose stellar content can be resolved with the modern detectors.

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