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- W3105556382 abstract "We use the two-point correlation function to calculate the clustering properties of the recently completed SSRS2 survey, which probes two well-separated regions of the sky, allowing one to evaluate the sensitivity of sample-to-sample variations. Taking advantage of the large number of galaxies in the combined sample, we also investigate the dependence of clustering on the internal properties of galaxies. The redshift-space correlation function for the combined magnitude-limited sample of the SSRS2 is given by ξ(s) = [s/(5.85 h-1 Mpc)]-1.60 for separations in the range 2 h-1 Mpc ≤ s ≤ 11 h-1 Mpc, while our best estimate for the real-space correlation function is ξ(r) = [r/(5.36 h-1 Mpc)]-1.86. Both are comparable with previous measurements using surveys of optical galaxies over much larger and independent volumes. By comparing the correlation function calculated in redshift and real space, we find that the redshift distortion on intermediate scales is small. This result implies that the observed redshift-space distribution of galaxies is close to that in real space and that β = Ω0.6/b < 1, where Ω is the cosmological density parameter and b is the linear biasing factor for optical galaxies." @default.
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- W3105556382 date "1998-03-01" @default.
- W3105556382 modified "2023-10-17" @default.
- W3105556382 title "Southern Sky Redshift Survey: Clustering of Local Galaxies" @default.
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- W3105556382 doi "https://doi.org/10.1086/300254" @default.
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