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Measuring our Universe from Galaxy Redshift Surveys.

作者信息

Lahav Ofer, Suto Yasushi

机构信息

Department of Physics and Astronomy, University of London, Gower Street, London, WC1E 6BT UK ; Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA UK.

Department of Physics and Research Center for the Early Universe, The University of Tokyo, Tokyo, 113-0033 Japan.

出版信息

Living Rev Relativ. 2004;7(1):8. doi: 10.12942/lrr-2004-8. Epub 2004 Jul 16.

DOI:10.12942/lrr-2004-8
PMID:28163643
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5253994/
Abstract

Galaxy redshift surveys have achieved significant progress over the last couple of decades. Those surveys tell us in the most straightforward way what our local Universe looks like. While the galaxy distribution traces the side of the Universe, detailed quantitative analyses of the data have even revealed the side of the Universe dominated by non-baryonic dark matter as well as more mysterious dark energy (or Einstein's cosmological constant). We describe several methodologies of using galaxy redshift surveys as cosmological probes, and then summarize the recent results from the existing surveys. Finally we present our views on the future of redshift surveys in the era of precision cosmology.

摘要
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