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.
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3 Pith papers cite this work, alongside 1 external citations. Polarity classification is still indexing.
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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.
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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.
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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.
- VERSUS: An excursion-set-inspired void-finder for the Stage-IV era