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This is the repository of final year project. This may include research based work. Please do not use results without proper citations.
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Final_Year_Project

This is the repository of final year project. This may include research based work. Please do not use results without proper citations.

Authors:Dr. Dasgupta K, Hari A,Dutta KK, Roy NG, Chowdhury PN. Institute: Kalyani Government Engineering College

The following image is after using kMeans (self implemented, as the kMeans algorithm needed to be modified to work on N-dimensions instead of 2 dimensions, which various packages generally implement) on the cloud dust of Kepler after supernova explosion: Image after processing

This image is then seperated into various clusters giving the following image. The following image the tries to show the boundary of various regions. It still needs some refinement.

seperate clusters

The credit for raw x-ray images:

  1. NASA/CXC/NCSU/K.Borkowski et al.
  2. NASA/CXC/NCSU/S. Reynolds et al.
  3. NASA/CXC/MIT/D. Dewey et al & NASA/CXC/SAO/J. DePasquale

We are extremely thankful to the authorities and research teams to make these images available to be used in our study.

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