发表机构
Space Telescope Science Institute; Johns Hopkins University; University of Arizona（太空望远镜科学研究所; 约翰斯·霍普金斯大学; 亚利桑那大学）
机构由 AI 辅助整理，请以论文原文为准。AI 中文总结
本文介绍JWST凭借独特能力在运行初期获得超新星观测成果，为超新星相关研究提供新窗口，将与未来罗曼空间望远镜互补推动超新星科学发展。
AI 中文摘要
超新星（SNe）是研究宇宙历史中星系的物理、化学及宇宙学环境的绝佳探针。詹姆斯·韦布空间望远镜（JWST）具备独特的波长覆盖范围、灵敏度和分辨率，自发射以来为超新星物理、前身星、尘埃产生、红移演化恒星种群及宇宙学研究提供了新的观测窗口。本文总结了JWST在运行最初几年对超新星开展的惊人观测成果，以及这些观测带来的宇宙认知进展，包括对近邻超新星的详细观测、首批高红移超新星的光谱样本，还有大量对宇宙学推断和高信噪比（S/N）光谱学均有重要价值的引力透镜超新星。尽管即将发射的南希·格蕾丝·罗曼空间望远镜有望彻底变革天基时域天文学，但JWST凭借其独特能力，将继续为各类超新星科学研究提供高精度光谱和测光数据，发挥互补作用。
英文摘要
Supernovae (SNe) are excellent probes of the physical, chemical, and cosmological context of galaxies across the history of the Universe. The James Webb Space Telescope (JWST ) has a truly unique combination of wavelength, sensitivity, and resolution, providing a new window into SN physics, progenitors, dust production, redshift evolving stellar populations, and cosmology since its launch. Here we summarize the astounding observations JWST has made of SNe in its first few years of operations, as well as the corresponding advancements in our understanding of the Universe. This includes detailed views of nearby SNe, the first spectroscopic samples of high-z SNe, and a significant number of gravitationally lensed SNe valuable for both cosmological inference and high signal-to-noise (S/N) spectroscopy. While the upcoming Nancy Grace Roman Space Telescope is expected to revolutionize space-based time-domain astronomy, JWST and its unique capabilities will continue to play a complementary role by providing high-precision spectroscopic and photometric data for a broad range of SN science cases.
CommentsFocus point special issue
Journal refPierel, J., Coulter, D., DeCoursey, C., et al. 2026, EPJ Plus, 141, 1155
DOI：10.1140/epjp/s13360-026-08293-1
