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GRB 050904のz = 6.39 +/- 0.12のフォトメトリック赤偏移は,GRB 050904のために

J B Haislip1, M C Nysewander, D E Reichart

  • 1Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Campus Box 3255, Chapel Hill, North Carolina 27599, USA.

Nature
|March 10, 2006
PubMed
まとめ

私たちは,赤道移転 z = 6.3 で,ガンマ線爆発 (GRB) の余光を発見しました.これらの宇宙イベントの記録です. この発見は,GRBが初期の宇宙を研究するための強力なツールであることを示しています.

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