Large-scale structure in the H I Parkes All-Sky Survey: filling the voids with H I galaxies?

2007/03/28 by S. Basilakos, Spyros Basilakos, M. Plionis +3 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Galaxies: Formation, Evolution, Phenomena #astro-ph

paper · pdf · doi:10.1111/j.1365-2966.2007.11781.x

published as Mon.Not.Roy.Astron.Soc.378:301-308,2007 · 9 pages, 8 figures, MNRAS in press

arxiv created 2007/03/28 · openalex publication_date 2007/05/10 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The clustering of the different extragalactic sources is an ideal tool for testing theories of structure formation as well as studying the large-scale structure (eg. Peebles 1993). The traditional indicator of clustering, the

Citations

• The HIPASS catalogue: ΩH i and environmental effects on the H i mass function of galaxies
• Cross-correlation of Lyman absorbers with gas-rich galaxies
• A Large Structure of Galaxies At Redshift z~3 and its Cosmological Implications
• The Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift 6
• Evolution of galaxy clustering
• DAMPED LYα SYSTEMS
• Ionization Properties and Elemental Abundances in Damped Lyα Systems

Cited by

• The Aspen–Amsterdam void finder comparison project