Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
Youcai Zhang, Volker Springel, Xiaohu Yang

TL;DR
This paper introduces a novel Delaunay tessellation method for analyzing the topology of cosmic large-scale structures, outperforming traditional smoothing techniques in extracting topological information from galaxy distributions.
Contribution
The paper presents a new Delaunay tessellation field estimation method for genus statistics, enabling precise topology measurement without free parameters and improving discrimination between galaxy catalogues.
Findings
Delaunay-based method captures more topological information.
It distinguishes between different galaxy catalogues effectively.
Detects discrepancies between models and SDSS data.
Abstract
We study the topology of cosmic large-scale structure through the genus statistics, using galaxy catalogues generated from the Millennium Simulation and observational data from the latest Sloan Digital Sky Survey Data Release (SDSS DR7). We introduce a new method for constructing galaxy density fields and for measuring the genus statistics of its isodensity surfaces. It is based on a Delaunay tessellation field estimation (DTFE) technique that allows the definition of a piece-wise continuous density field and the exact computation of the topology of its polygonal isodensity contours, without introducing any free numerical parameter. Besides this new approach, we also employ the traditional approaches of smoothing the galaxy distribution with a Gaussian of fixed width, or by adaptively smoothing with a kernel that encloses a constant number of neighboring galaxies. Our results show that…
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