An Analysis of SDSS Data Using the Galaxy Anisotropic Correlation Function

Details An Analysis of SDSS Data Using the Galaxy Anisotropic Correlation Function An Analysis of SDSS Data Using the Galaxy Anisotropic Correlation Function

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008asthe.101..589o&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 101, No. 10, p. 589 - 597 (2008)

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Recent observation such as the cosmic microwave background, Type Ia supernovae, and large-scale structure of the universe, constrained cosmological parameters with high precision. A cosmological analysis through galaxy distributions from the Sloan Digital Sky Survey is reviewed. Constraints on cosmological parameters including the dark energy using the anisotropic correlation function in redshift space are also presented.

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