The galaxies, are the systems consisting of
stars, gas, dust and dark matter combined with the gravitational force. There
are billions of galaxies in the universe. Since the cost of examining each
galaxy one by one is high, the classification of the galaxy is an important
part of the astronomical data analysis. Galaxies are classified according to
morphology and spectral properties. Machine learning methods aimed at revealing
the hidden pattern within the data set by analyzing the available data, it can
be used to estimate which group of galaxies whose natural groups have not yet
been identified. This will save time and cost for both researchers and
astronomers. This study has been classified five-variables (Right ascension,
Declination, Magnitude, Velocity, and Sigma of Velocity) 4215 galaxies.
Galaxies whose natural groups were determined with IDL were classified by using
machine learning algorithms with Weka program. Bayes classifier methods, Naive
Bayes and Bayes net, Decision tree methods J48, LMT and Random Forest
algorithms, Artificial Neural Networks Multilayer Perceptron and Support vector
classifier methods were used. The obtained classification results were compared
with the natural groups and the predictive performance of the methods were
evaluated.
Galaxies Classification Classification Algorithms Machine Learning Shapley Concentration Region
Birincil Dil | İngilizce |
---|---|
Konular | Mühendislik |
Bölüm | Makaleler |
Yazarlar | |
Yayımlanma Tarihi | 30 Haziran 2019 |
Yayımlandığı Sayı | Yıl 2019 Cilt: 5 Sayı: 1 |