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arXiv:astro-ph/9410068 (astro-ph)
[Submitted on 20 Oct 1994]

Title:Constraints on Cosmological Models from Once and Future Redshift Surveys

Authors:Michael S. Vogeley
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Abstract: The power spectrum of density fluctuations measured from galaxy redshift surveys provides important constraints on models for the formation of large-scale structure. I present new results for a redshift sample of 15,000 galaxies, and review the limitations of current measurements. To span the decade of wavelength between the scales probed by galaxy surveys and COBE, measure the detailed shape of the power spectrum, and accurately examine the dependence of clustering on galaxy species, we require deeper samples with carefully controlled selection criteria and improved techniques for power spectrum estimation. I review plans for the Sloan Digital Sky Survey and describe a new method for estimating the power spectrum that optimally treats survey data with arbitrary geometry and sampling.
Comments: To appear in Wide-Field Spectroscopy and the Distant Universe, eds. S. J. Maddox and A. Aragon-Salamanca (World Scientific: Singapore); Proc. of 35th Herstmonceux Conference, Cambridge, U.K., July 4-8, 1994. 15 pages uuencoded compressed postscript, including 7 figures. JHU-94102002
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/9410068
  (or arXiv:astro-ph/9410068v1 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/9410068

Submission history

From: Michael Vogeley [view email]
[v1] Thu, 20 Oct 1994 17:45:10 UTC (226 KB)
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