Understanding the birth and evolution of galaxies, and the history of star formation in them, is one of the most important problems in astronomy. Using the data from the AKARI IRC survey of the Large Magellanic Cloud at 3.2, 7, 11, 15, and 24 μm , we have constructed a multi-wavelength catalog containing data from the cross-correlation with a number of other databases at different wavelengths. We present the first approach with a Support Vector Machine (SVM)-based method to separate different classes of stars in LMC in the color-color and color-magnitude diagrams.

ABSTRACT
1. INTRODUCTION
2. COLOR-MAGNITUDE DIAGRAMS
REFERENCES

• M. SIUDEK(Centre for Theoretical Physics of the Polish Academy of Sciences)
• A. POLLO(Centre for Theoretical Physics of the Polish Academy of Sciences, Astronomical Observatory of the Jagiellonian University, National Centre for Nuclear Research)
• T. T. TAKEUCHI(Division of Particle and Astrophysical Science, Nagoya University)
• Y. ITA(Astronomical Institute, Tohoku University)
• D. KATO(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
• T. ONAKA(Department of Astronomy, The University of Tokyo)