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Finding Clusters of Galaxies in the Sloan Digital Sky Survey using Voronoi Tessellation
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Finding Clusters of Galaxies in the Sloan Digital Sky Survey using Voronoi Tessellation

Rita S. J Kim, Michael A Strauss, Neta A Bahcall, James E Gunn, Robert H Lupton, Wolfgang Voges, Michael S Vogeley and David Schlegel
ArXiv.org
15 Dec 1999
url
https://doi.org/10.48550/arxiv.astro-ph/9912302View
Preprint (Author's original)arXiv.org - Non-exclusive license to distribute Open

Abstract

Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics
The Sloan Digital Sky Survey has obtained 450 square degrees of photometric scan data, in five bands (u',g',r',i',z'), which we use to identify clusters of galaxies. We illustrate how we do star-galaxy separation, and present a simple and elegant method of detecting overdensities in the galaxy distribution, using the Voronoi Tessellation.

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