eROSITA를 이용한 대마젤란운의 초신성 잔해 집단에 대한 첫 번째 연구
본 논문에서는 eROSITA X선 망원경의 첫 4회 전천 탐사 데이터(eRASS:4)를 사용하여 대마젤란운(LMC)에서 초신성 잔해(SNR)의 최신 목록을 제시하고, 다파장 관측을 통해 새로운 SNR 후보를 식별하고 특징을 분석합니다.
大マゼラン雲の超新星残骸集団に関するeROSITAを用いた初の研究
本稿では、eROSITAのX線全天サーベイデータを用いて、大マゼラン雲（LMC）における超新星残骸（SNR）の集団を包括的に調査し、新たなSNR候補を特定し、既知のSNRの特性を分析することで、銀河の進化におけるSNRの役割の理解を深めることを目的とする。
First Study of the Supernova Remnant Population in the Large Magellanic Cloud with eROSITA: Identifying Supernova Remnants Using X-ray, Optical, and Radio Data
This research leverages the eROSITA X-ray telescope to conduct a comprehensive study of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC), utilizing multi-wavelength data analysis to identify and characterize these objects.
Predicting the Detectability of Supernova Remnants Using the Southern Wide-field Gamma-ray Observatory
This research paper presents a model for predicting the detectability of supernova remnants (SNRs) using the Southern Wide-field Gamma-ray Observatory (SWGO), highlighting its potential to identify new SNRs and contribute to our understanding of cosmic ray origins.
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