Direct Detection of Type II-P Supernova Progenitors with the Euclid and CSST Surveys

arXiv:2601.10121 · astro-ph.SR, astro-ph.HE · Submitted 2026-01-15 · Read on arXiv

astro-ph.SR, astro-ph.HE

Submitted: 2026-01-15

Updated: 2026-08-31

Comments: 12 pages, 8 figures, accepted by SCPMA

DOI: 10.1007/s11433-026-3104-9

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

Terminology

• Metallicity — 3× in this paper · explained in 3 episodes
• Robustness — 2× in this paper · explained in 5 episodes
• China Space Station — 1× in this paper
• Chinese Space-station Survey Telescope — 1× in this paper
• Consistency — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• Elias — 1× in this paper · explained in 2 episodes
• Hubble Space Telescope — 1× in this paper
• Markov Chain Monte Carlo — 1× in this paper
• National Natural Science Foundation of China — 1× in this paper
• Near Infrared Spectrometer and Photometer — 1× in this paper
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes

Sources

• Mock Observations for the CSST Mission: Main Surveys--An Overview of Framework and Simulation Suite
• Mock Observations for the CSST Mission: End-to-End Performance Modeling of Optical System
• Introduction to the Chinese Space Station Survey Telescope (CSST)

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