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We propose observations of new supernova remnant (SNR) candidates in the LargeMagellanic Cloud (LMC). Building on a successful campaign to observe candidateswith ROSAT detections we now propose observations of the lowest X-ray surfacebrightness SNR candidates which were found in the newest eROSITA data andconfirmed in multi-wavenlength observations. The high sensitivity of XMM-Newtonwill allow us to confirm SNRs at the faintest end of the X-ray luminosityfunction (XLF) and study their plasma properties and age as well as the ambientinterstellar medium (ISM). [truncated! Please see actual data for full text]

本研究提出针对大麦哲伦星系（Large Magellanic Cloud, LMC）内新的超新星遗迹（supernova remnant, SNR）候选体的观测计划。依托此前利用伦琴X射线卫星（ROSAT）探测候选体并取得成功的观测项目，我们此次提出针对最新eROSITA数据中发现、且经多波段观测验证的低X射线面亮度超新星遗迹候选体的观测计划。XMM-牛顿望远镜（XMM-Newton）的高灵敏度将使我们能够确认处于X射线光度函数（X-ray luminosity function, XLF）最暗端的超新星遗迹，并研究其等离子体特性、年龄以及周围星际介质（interstellar medium, ISM）的性质。【文本已截断！完整内容请查阅原始数据集】