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A New Method to Classify Type IIP/IIL Supernovae Based on their Spectra
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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.
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Cited by 1 Pith paper
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On the photometric and spectroscopic diversity of Type II supernovae
Type II supernova diversity is best explained by a combination of reduced hydrogen envelope mass and a confined circumstellar shell, with fast decliners requiring 0.5 to 1 solar mass of circumstellar material.
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