English

A New Method to Classify Type IIP/IIL Supernovae Based on their Spectra

High Energy Astrophysical Phenomena 2018-11-08 v1

Abstract

Type IIP and type IIL supernovae (SNe) are defined on their light curves, but the spectrum criteria in distinguishing these two type SNe remains unclear. We propose a new classification method. Firstly, we subtract the principal components of different wavelength bands in the spectra based on Functional Principal Components Analysis (FPCA) method. Then, we use Support Vector Machine (SVM) and Artificial Neural Network (ANN) to classify these two types of SNe. The best F1-Score of our classifier is 0.881, and we found that solely using Halpha line at 6150-6800 A for classification can reach a F1-Score up to 0.849. Our result indicates that the profile of the Halpha is the key to distinguish the two type SNe.

Keywords

Cite

@article{arxiv.1811.03022,
  title  = {A New Method to Classify Type IIP/IIL Supernovae Based on their Spectra},
  author = {Xingzhuo Chen and Shihao Kou and Xuewen Liu},
  journal= {arXiv preprint arXiv:1811.03022},
  year   = {2018}
}

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R2 v1 2026-06-23T05:08:00.478Z