サイエンス
史上最も強力なガンマ線バーストは超新星によって引き起こされたことがJWSTのデータで確認される
約20億年の旅を経て、2022年10月9日、極めて高エネルギーのガンマ線バースト（GRB）からの光子が、ニール・ゲールズ・スウィフト天文台とフェルミ・ガンマ線宇宙望遠鏡のセンサーに衝突した。GRBは7分間続いたが、もっと […]
Overview
最終更新: 2026年6月10日The Neil Gehrels Swift Observatory is a NASA space telescope designed to detect gamma-ray bursts (GRBs). Launched in 2004, it is equipped with three instruments that work together to observe GRBs and their afterglows in gamma-ray, X-ray, ultraviolet, and optical wavebands. Its rapid response capability allows it to slew and point at a new burst within seconds of detection.
Mentioned Articles
1 件External Mentions
6 件- arXiv Probing dipole and quadrupole anisotropy in Gamma-ray bursts from Swift dataset
- arXiv The SVOM mission, its profile and its system
- arXiv Rapid-response 1.3 mm Observations of GRB 260127A with the Submillimeter Array
- arXiv Multi-mission Investigation of X-ray Superorbital Modulation in the Supergiant High Mass X-ray Binary 4U 1538-52
- arXiv Superorbital Phase Evolution and a Soft-Hard X-ray Phase Shift in LMC X-4
- arXiv The Double-Burst Nature and Early Afterglow Evolution of Long GRB 110801A