UNSUPERVISED CLUSTERING OF TYPE II SUPERNOVA LIGHT CURVES

Adam Rubin, Avishay Gal‐Yam

The Astrophysical Journal 2016 article cited by 42

importance 4/10 ai assisted Gamma-ray bursts and supernovae astronomy stage: research

Astronomers needed a systematic, unbiased way to classify Type II supernova light curves ahead of upcoming large transient surveys.

Systematic classification of supernova light curves underpins understanding of stellar explosions and handling of future extremely large data sets.

Unsupervised k-means clustering was applied to 59 R-band SN II light curves, showing the rise-to-peak phase matters and dividing the sample into three classes plus three outliers.

Sample divided into three classes (II-S, II-FS, II-FF) with three outliers; II-FS significantly less luminous; II-S bridges the gap between II-P/II-L populations.

The clustering result offered an explanation for recent conflicting findings on II-P/II-L populations.

Venue The Astrophysical Journal
Published 2016
Work type article
Authors Adam Rubin, Avishay Gal‐Yam
Citations 42 (OpenAlex, at import time)
References 21
Model or method k-means clustering (with principal component analysis)
Organization not stated in source
Primary source https://doi.org/10.3847/0004-637x/828/2/111
Open access bronze
Keywords supernovae, light curves, k-means, unsupervised clustering, transients
4 / 10

real but narrower advance

Systematic SN II light-curve classification ahead of extremely large transient surveys; foundational astronomy but narrow specific problem.

Basis: inferred. Judged from the source text, which gives no explicit scale. Stated scale: 59 R-band SN II light curves. Method and limits.

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