Year: 1995
Type: article
Abstract: Under the assumption of a void-filled Universe we investigate whether the characteristic scale of voids can be determined from existing surveys. We use the Voronoi tessellation to create mock surveys and study the properties of the first zero-crossing of the two-point correlation function for various survey geometries. Our main conclusion is that the available data sets should be able to discriminate between 5000 km s-1 and 12000 km s-1 voids, if one of these scales actually characterizes the distribution of galaxies.
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W1977364995
