Large-Scale Structure and Future Surveys
| dc.creator | Eisenstein, Daniel | |
| dc.date | 2003-01-30 | |
| dc.date.accessioned | 2026-07-07T02:07:24Z | |
| dc.date.available | 2026-07-07T02:07:24Z | |
| dc.description | 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. | |
| dc.description | Proceedings from Wide-Field Multi-Object Spectroscopy conference at NOAO in October 2001, to be published by the ASP Conference Series. 8 pages, LaTex, 1 figure | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0301623 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0301623 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5682 | |
| dc.subject | Astrophysics | |
| dc.title | Large-Scale Structure and Future Surveys | |
| dc.type | text |