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The Korean Astronomical Society (한국천문학회)
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INFRARED COMPOSITION OF THE LARGE MAGELLANIC CLOUD

  • Siudek, M. (Centre for Theoretical Physics of the Polish Academy of Sciences) ;
  • Pollo, A. (Centre for Theoretical Physics of the Polish Academy of Sciences) ;
  • Takeuchi, T.T. (Division of Particle and Astrophysical Science, Nagoya University) ;
  • Ita, Y. (Astronomical Institute, Tohoku University) ;
  • Kato, D. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Onaka, T. (Department of Astronomy, The University of Tokyo)
  • Received : 2012.06.20
  • Accepted : 2012.07.23
  • Published : 2012.09.16
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Abstract

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 $24{\mu}m$, 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.

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References

  1. Chang, C. C. & Lin, C. J., 2011, LIBSVM: A Library for Support Vector Machines. ACM TIST, 2:27:127:27
  2. Ita, Y., et al., 2008, AKARI IRC Survey of the Large Magellanic Cloud: Outline of the Survey and Initial Results, PASJ, 60, 435