Photometric classification of Hyper Suprime-Cam transients using machine learning
Abstract
Abstract The advancement of technology has resulted in a rapid increase in supernova (SN) discoveries. The Subaru/Hyper Suprime-Cam (HSC) transient survey, conducted from fall 2016 through spring 2017, yielded 1824 SN candidates. This gave rise to the need for fast type classification for spectroscopic follow-up and prompted us to develop a machine learning algorithm using a deep neural network with highway layers. This algorithm is trained by actual observed cadence and filter combinations such that we can directly input the observed data array without any interpretation. We tested our model with a dataset from the LSST classification challenge (Deep Drilling Field). Our classifier scores an area under the curve (AUC) of 0.996 for binary classification (SN Ia or non-SN Ia) and 95.3% accuracy for three-class classification (SN Ia, SN Ibc, or SN II). Application of our binary classification to HSC transient data yields an AUC score of 0.925. With two weeks of HSC data since the first detection, this classifier achieves 78.1% accuracy for binary classification, and the accuracy increases to 84.2% with the full dataset. This paper discusses the potential use of machine learning for SN type classification purposes.
- Authors:
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1657872
- Resource Type:
- Published Article
- Journal Name:
- Publications of the Astronomical Society of Japan
- Additional Journal Information:
- Journal Name: Publications of the Astronomical Society of Japan Journal Volume: 72 Journal Issue: 5; Journal ID: ISSN 0004-6264
- Publisher:
- Oxford University Press
- Country of Publication:
- Japan
- Language:
- English
Citation Formats
Takahashi, Ichiro, Suzuki, Nao, Yasuda, Naoki, Kimura, Akisato, Ueda, Naonori, Tanaka, Masaomi, Tominaga, Nozomu, and Yoshida, Naoki. Photometric classification of Hyper Suprime-Cam transients using machine learning. Japan: N. p., 2020.
Web. doi:10.1093/pasj/psaa082.
Takahashi, Ichiro, Suzuki, Nao, Yasuda, Naoki, Kimura, Akisato, Ueda, Naonori, Tanaka, Masaomi, Tominaga, Nozomu, & Yoshida, Naoki. Photometric classification of Hyper Suprime-Cam transients using machine learning. Japan. https://doi.org/10.1093/pasj/psaa082
Takahashi, Ichiro, Suzuki, Nao, Yasuda, Naoki, Kimura, Akisato, Ueda, Naonori, Tanaka, Masaomi, Tominaga, Nozomu, and Yoshida, Naoki. Fri .
"Photometric classification of Hyper Suprime-Cam transients using machine learning". Japan. https://doi.org/10.1093/pasj/psaa082.
@article{osti_1657872,
title = {Photometric classification of Hyper Suprime-Cam transients using machine learning},
author = {Takahashi, Ichiro and Suzuki, Nao and Yasuda, Naoki and Kimura, Akisato and Ueda, Naonori and Tanaka, Masaomi and Tominaga, Nozomu and Yoshida, Naoki},
abstractNote = {Abstract The advancement of technology has resulted in a rapid increase in supernova (SN) discoveries. The Subaru/Hyper Suprime-Cam (HSC) transient survey, conducted from fall 2016 through spring 2017, yielded 1824 SN candidates. This gave rise to the need for fast type classification for spectroscopic follow-up and prompted us to develop a machine learning algorithm using a deep neural network with highway layers. This algorithm is trained by actual observed cadence and filter combinations such that we can directly input the observed data array without any interpretation. We tested our model with a dataset from the LSST classification challenge (Deep Drilling Field). Our classifier scores an area under the curve (AUC) of 0.996 for binary classification (SN Ia or non-SN Ia) and 95.3% accuracy for three-class classification (SN Ia, SN Ibc, or SN II). Application of our binary classification to HSC transient data yields an AUC score of 0.925. With two weeks of HSC data since the first detection, this classifier achieves 78.1% accuracy for binary classification, and the accuracy increases to 84.2% with the full dataset. This paper discusses the potential use of machine learning for SN type classification purposes.},
doi = {10.1093/pasj/psaa082},
journal = {Publications of the Astronomical Society of Japan},
number = 5,
volume = 72,
place = {Japan},
year = {Fri Sep 04 00:00:00 EDT 2020},
month = {Fri Sep 04 00:00:00 EDT 2020}
}
https://doi.org/10.1093/pasj/psaa082
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