VERSUS is a void-finding algorithm that identifies spherical underdensities matching excursion-set predictions for the void size function, validated on synthetic particles and AbacusSummit mocks with realistic galaxy populations.
Title resolution pending
4 Pith papers cite this work, alongside 162 external citations. Polarity classification is still indexing.
4
Pith papers citing it
162
external citations · OpenAlex
years
2026 4representative citing papers
Void galaxies identified by local volume in non-spherical voids are bluer and more star-forming than non-void galaxies, with the environmental effect decreasing with stellar mass.
A catalogue of 37 voids (radii 13-38 h^{-1} Mpc) and 42 knots (volumes 10^4 to 3.3x10^5 h^{-3} Mpc^3) is presented using V-web on CF4++ZOA peculiar velocities within z=0.1.
Group-voids identified from galaxy group catalogs reproduce halo-void size functions and density profiles in CSST mocks above ~40% spectroscopic completeness, with incompleteness at 30% captured by an effective redshift-error parameter.
citing papers explorer
-
VERSUS: An excursion-set-inspired void-finder for the Stage-IV era
VERSUS is a void-finding algorithm that identifies spherical underdensities matching excursion-set predictions for the void size function, validated on synthetic particles and AbacusSummit mocks with realistic galaxy populations.
-
Quantifying Environmental Effects on Galaxy Properties using Non-spherical Voids Identified from SDSS DR7
Void galaxies identified by local volume in non-spherical voids are bluer and more star-forming than non-void galaxies, with the environmental effect decreasing with stellar mass.
-
A local Universe catalogue of structures and voids dynamically identified using Cosmic-Flows4++ZOA peculiar velocities
A catalogue of 37 voids (radii 13-38 h^{-1} Mpc) and 42 knots (volumes 10^4 to 3.3x10^5 h^{-3} Mpc^3) is presented using V-web on CF4++ZOA peculiar velocities within z=0.1.
-
CSST large-scale structure analysis pipeline: IV. Cosmic Voids Identified from Galaxy Group Samples as Probes of the Large-scale Structure
Group-voids identified from galaxy group catalogs reproduce halo-void size functions and density profiles in CSST mocks above ~40% spectroscopic completeness, with incompleteness at 30% captured by an effective redshift-error parameter.