Automated Clustering Algorithms for Classification of Astronomical Objects
arXiv:astro-ph/0403431 · doi:10.1051/0004-6361:20040141
Abstract
Data mining is an important and challenging problem for the efficient analysis of large astronomical databases and will become even more important with the development of the Global Virtual Observatory. In this study, learning vector quantization (LVQ), single-layer perceptron (SLP) and support vector machines (SVM) were put forward for multi-wavelength data classification. A feature selection technique was used to evaluate the significance of the considered features to the results of classification. From the results, we conclude that in the situation of less features, LVQ and SLP show better performance. In contrast, SVM shows better performance when considering more features. The focus of the automatic classification is on the development of efficient feature-based classifier. The classifiers trained by these methods can be used for preselecting AGN candidates.
Accepted for publication in A&A
References in corpus (10)
- The Identification of EGRET Sources with Flat-Spectrum Radio Sources
- AUTOMATED MORPHOLOGICAL CLASSIFICATION OF APM GALAXIES BY SUPERVISED ARTIFICIAL NEURAL NETWORKS
- Automated Classification of Stellar Spectra. II: Two-Dimensional Classification with Neural Networks and Principal Components Analysis
- An Artificial Neural Network Approach to Classification of Galaxy Spectra
- Neural computation as a tool for galaxy classification : methods and examples
- Identification of selected sources from the ROSAT Galactic Plane Survey - I
- Wide Field Imaging. I. Applications of Neural Networks to object detection and star/galaxy classification
- XID: Cross-Association of ROSAT/Bright Source Catalog X-ray Sources with USNO A2 Optical Point Sources
- The INT Search for Metal-Poor Stars. Spectroscopic Observations and Classification via Artificial Neural Networks
- Automated Source Classification using a Kohonen Network
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