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Updated: May 1, 2026

Hyperspectral Imaging as a Tool to Study Optical Anisotropy in Lanthanide-Based Molecular Single Crystals
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近赤外線背景アニソトロピーは,銀河の拡散したイントラハロ光によるものです

Asantha Cooray1, Joseph Smidt, Francesco De Bernardis

  • 1Department of Physics and Astronomy, University of California, Irvine, California 92697, USA. acooray@uci.edu

Nature
|October 27, 2012
PubMed
まとめ

宇宙近赤外線背景アニソトロピーは,初期の銀河や矮星銀河から発生している可能性があります. 新しい測定は,より大きなクラスタリング振幅を明らかにし,銀河内のイントラハロ星が赤道シフト1〜4の主要な寄与者であることを示唆しています.

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