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Large-Scale Structure and Future Surveys

Daniel Eisenstein
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Abstract

As 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.

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Daniel Eisenstein. 2003-01-30. Large-Scale Structure and Future Surveys. https://arxiv.org/abs/astro-ph/0301623

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