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STag: Supernova Tagging and Classification

delete2022-02-04
delete3
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OA
AI
W
William Davison
D
David Parkinson *
B
B. Tucker
DOI:10.3847/1538-4357/ac3422delete
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摘要

摘要

En 中文
Supernovae classes have been defined phenomenologically, based on spectral features and time series data, since the specific details of the physics of the different explosions remain unrevealed. However, the number of these classes is increasing as objects with new features are observed, and the next generation of large surveys will only bring more variety to our attention. We apply the machine learning technique of multi-label classification to the spectra of supernovae. By measuring the probabilities of specific features or tags in the supernova spectra, we can compress the information from a specific object down to that suitable for a human or database scan, without the need to directly assign to a reductive class. We use logistic regression to assign tag probabilities, and then a feed-forward neural network to filter the objects into the standard set of classes, based solely on the tag probabilities. We present STag, a software package that can compute these tag probabilities and make spectral classifications.
Keyword:
ELECTRON-CAPTURE SUPERNOVAE
CORE-COLLAPSE
DATA REDUCTION
IA PROGRAM
REDSHIFT
SPECTROSCOPY
EVOLUTION
SPECTRA
II.

期刊

Astrophysical Journal 封面图
Astrophysical Journal
IF:
5.4
论文数:
8.3W
被引数:
32.0W

机构

K
korea astronomy & space science institute (kasi)
学者数:
1.8K
论文数: 2.1K
被引数: 3
A
Australian National University
学者数:
2.1W
论文数: 2.3W
被引数: 3.9W
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