The Topology of the Las Campanas Redshift Survey as Assessed by Percolation Analysis

Details The Topology of the Las Campanas Redshift Survey as Assessed by Percolation Analysis The Topology of the Las Campanas Redshift Survey as Assessed by Percolation Analysis

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...19513701y&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #137.01; Bulletin of the American Astronomical Society, Vol. 32, p.884

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a review of the Percolation Analysis of the Las Campanas Redshift Survey including an unpublished assessment of the 3-D topology. Percolation analysis has been developed, over the last decade, as a sensitive tool for describing the topology of galaxy distributions in astronomical surveys. The analysis can distinguish between clumpy and connected distributions of galaxies for surveys that have very different geometries or selection criteria. The topology of galaxy distributions has implications for theories of large-scale structure development.

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