A Percolation Analysis of the Topology of the Las Campanas Redshift Survey

Details A Percolation Analysis of the Topology of the Las Campanas Redshift Survey A Percolation Analysis of the Topology of the Las Campanas Redshift Survey

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...191.6302y&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #63.02; Bulletin of the American Astronomical Society, Vol. 29, p.1309

Astronomy and Astrophysics

Astronomy

Scientific paper

In the past decade, percolation analysis has developed into a powerful and sensitive tool for describing the topology of mass and galaxy distributions. The analysis can distinguish between isolated (clumpy) and connected (filamentary) distributions of galaxies. In this paper, we present a percolation analysis of the Las Campanas Redshift Survey. This work has implications for the local isotropy of the universe and the evolution of large-scale structure.

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