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Las Campanas Redshift Survey : ウィキペディア英語版 | Las Campanas Redshift Survey The Las Campanas Redshift Survey is considered the first attempt to map a large area of the universe out to a redshift of ''z'' = 0.2. It was begun in 1991 using the Las Campanas telescope in Chile to catalog 26418 separate galaxies.〔(Las Campanas Redshift Survey web page )〕 It is considered one of the first surveys to document the so-called "end of greatness" where the Cosmological Principle of isotropy could be seen. Superclusters and voids are prominent features in the survey. ==References==
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Las Campanas Redshift Survey」の詳細全文を読む
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