천문학회보 (The Bulletin of The Korean Astronomical Society)
- 제42권2호
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- Pages.64.3-64.3
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- 2017
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- 1226-2692(pISSN)
Feature engineering with Wavelet transform for Transient detection in KMTNet Supernova Project
초록
For the detection of transient sources in optical wide field surveys like KMTNet Supernova Project, difference imaging technique is commonly used. As this method produces a fair amount of false positives, it is also common to utilize machine learning algorithms to screen likely true positives. While deep learning methods such as a convolutional neural network has been successfully applied recently, its application can be limited if the size of the training sample is small. I will discuss a variation of more conventional method that adopts the wavelet transform for feature engineering and its performance.
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