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Updated: May 10, 2026

Angle-resolved Photoemission Spectroscopy At Ultra-low Temperatures
08:53

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Published on: October 9, 2012

銀河の異常なスペクトルエネルギー分布は,以前は赤偏移6.68と報告されていた

H W Chen1, K M Lanzetta, S Pascarelle

  • 1Observatories of the Carnegie Institution of Washington, Pasadena, California 91101, USA. hchen@ociw.edu

Nature
|December 16, 2000
PubMed
まとめ

初期の銀河を特定することは困難です. 新しい光度測定データは,赤道偏移z=6.68の銀河についての以前の発見と矛盾しており,その赤道偏移と性質は未定である.

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