The VIMOS VLT deep survey: testing the gravitational instability paradigm at z ~ 1

2008/02/07 by C. Marinoni, L. Guzzo, A. Cappi +74 · 3 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078891

14 pages, 5 figures, A&A in Press

arxiv created 2008/02/13 · openalex publication_date 2008/08/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

14 pages, 5 figures, A&A in Press

Citations

• The Probability Distribution Function of Light in the Universe: Results from Hydrodynamic Simulations
• Probability Distribution Function of Cosmological Density Fluctuations from a Gaussian Initial Condition: Comparison of One‐Point and Two‐Point Lognormal Model Predictions withN‐Body Simulations
• Mapping the Universe

Cited by

• A null test of the metric nature of the cosmic acceleration
• Characterization of the distribution of the Llyαemitters in the 53W002 field at z = 2.4
• OBSERVATIONAL REQUIREMENTS FOR Lyα FOREST TOMOGRAPHIC MAPPING OF LARGE-SCALE STRUCTURE ATz∼ 2

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• Studying the Evolution of Multi-Wavelength Emissivities with the Vimos VLT Deep Survey
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• Very Large Array Sky Survey (VLASS) white paper: Go deep, not wide