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The VIMOS VLT Deep Survey : Testing the gravitational instability paradigm at z ∼ 1
We have reconstructed the three-dimensional density fluctuation maps to z ~ 1.5 using the distribution of galaxies observed in the VVDS-Deep survey. We use this overdensity field to measure the evolution of the probability distribution function and its lower-order moments over the redshift interval...
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Published in: | Astronomy and astrophysics (Berlin) 2008-08, Vol.487 (1), p.7-17 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites |
Online Access: | Get full text |
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Summary: | We have reconstructed the three-dimensional density fluctuation maps to z ~ 1.5 using the distribution of galaxies observed in the VVDS-Deep survey. We use this overdensity field to measure the evolution of the probability distribution function and its lower-order moments over the redshift interval 0.7 |
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ISSN: | 0004-6361 1432-0746 1432-0756 |
DOI: | 10.1051/0004-6361:20078891 |