The Cosmically Depressed: Life, Sociology and Identity of Voids

TL;DR

This paper reviews the formation, structure, and galaxy populations of cosmic voids, introducing a new tessellation-based method for identifying and analyzing voids in galaxy surveys to study their properties.

Contribution

It presents a novel parameter-free watershed technique for void detection in galaxy surveys, facilitating detailed analysis of void substructure and galaxy content.

Findings

Effective void detection in galaxy surveys using the new method

Identification of galaxies in the deepest cosmic troughs

Insights into void formation and hierarchical evolution

Abstract

We review and discuss aspects of Cosmic Voids that form the background for our Void Galaxy Survey (see accompanying paper by Stanonik et al.). Following a sketch of the general characteristics of void formation and evolution, we describe the influence of the environment on their development and structure and the characteristic hierarchical buildup of the cosmic void population. In order to be able to study the resulting tenuous void substructure and the galaxies populating the interior of voids, we subsequently set out to describe our parameter free tessellation-based watershed void finding technique. It allows us to trace the outline, shape and size of voids in galaxy redshift surveys. The application of this technique enables us to find galaxies in the deepest troughs of the cosmic galaxy distribution, and has formed the basis of our void galaxy program.