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20 April 2024
 
  » arxiv » astro-ph/0301623

 Article overview


Large-Scale Structure and Future Surveys
Daniel Eisenstein ;
Date 30 Dec 2002
Subject astro-ph
AffiliationSteward Observatory
AbstractAs the 2dF Galaxy Redshift Survey and Sloan Digital Sky Survey move toward completion, it is time to ask what the next generation of survey of large-scale structure should be. I discuss some of the cosmological justifications for such surveys and conclude that surveys at z=3 offer a critical advantage in their ability to access linear-regime clustering at scales smaller than any current survey and even the CMB. I discuss a possible implementation of such a survey and highlight some of the potential science return.
Source arXiv, astro-ph/0301623
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