1995/09/07 by Douglas Scott, D. Scott, Scott, Douglas
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9509035
9 pages, including 4 figures in a uuencoded self-unpacking shell script. To appear in Proceedings of the ASP Symposium: Clusters, Lensing and the Future, edited by Virginia Trimble
arxiv created 1995/09/07 · openalex publication_date 1995/09/07 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We are now beginning to learn detailed information about cosmological parameters from the shapes of the matter and radiation power spectra, together with their relative normalization. As more high quality data are gathered from galaxy surveys and from microwave anisotropies, the range of allowed models is expected to get incrementally smaller. The amount of information potentially available from a high-resolution satellite experiment should allow a determination of essentially \it all currently discussed cosmological parameters to less than ~10%.