How Low Can We Go? Minimum Spectroscopic Requirements For Supernova Subtype Classification

arXiv:2607.03532 · astro-ph.IM, astro-ph.HE, astro-ph.SR · Submitted 2026-07-03 · Read on arXiv

astro-ph.IM, astro-ph.HE, astro-ph.SR

Submitted: 2026-07-03

Updated: 2026-08-29

Comments: 21 pages, 7 figures

Code: https://github.com/FoxFortino/spec_res

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Core — 8× in this paper · explained in 2 episodes
Signal-to-noise ratio (SNR) — 4× in this paper · explained in 2 episodes
Transformer — 4× in this paper · explained in 2 episodes
Consistency — 2× in this paper · explained in 3 episodes
Data Augmentation — 2× in this paper · explained in 7 episodes
AGN — 1× in this paper · explained in 1 episode
Accuracy — 1× in this paper · explained in 1 episode
Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
Attention Mechanism — 1× in this paper · explained in 3 episodes
Data Provenance — 1× in this paper · explained in 2 episodes
Degeneracy — 1× in this paper · explained in 3 episodes
Homogeneity — 1× in this paper · explained in 2 episodes
Observatory Legacy Survey of Space and Time — 1× in this paper
Provenance — 1× in this paper · explained in 4 episodes
Robustness — 1× in this paper · explained in 5 episodes
Zwicky Transient Facility — 1× in this paper

Sources

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