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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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Bibliographic Details
Published in:Astronomy and astrophysics (Berlin) 2008-08, Vol.487 (1), p.7-17
Main Authors: MARINONI, C, GUZZO, L, DE LA TORRE, S, VIREY, J. M, BOTTINI, D, GARILLI, B, LE BRUN, V, MACCAGNI, D, PICAT, J. P, SCODEGGIO, M, TRESSE, L, VETTOLANI, G, CAPPI, A, ZANICHELLI, A, ADAMI, C, ARNOUTS, S, BARDELLI, S, BOLZONELLA, M, CHARIOT, S, CILIEGI, P, CONTINI, T, FOUCAUD, S, FRANZETTI, P, LE FEVRE, O, GAVIGNAUD, I, ILBERT, O, LAMAREILLE, F, MARANO, B, MATHEZ, G, MERIGHI, R, PALTANI, S, PELLBO, R, POZZETTI, L, RADOVICH, M, MAZURE, A, VERGANI, D, ZAMORANI, G, ZUCCA, E, ABBAS, U, BONDI, M, BONGIORNO, A, BRINCHMANN, J, BUZZI, A, CUCCIATI, O, DE RAVEL, L, MENEUX, B, GREGORINI, L, MELLIER, Y, MERLUZZI, P, PEREZ-MONTERO, E, TAXIL, P, TEMPORIN, S, WALCHER, C. J, POLLO, A, IOVINO, A, MCCRACKEN, H. J, SCARAMELLA, R
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Language:English
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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
ISSN:0004-6361
1432-0746
1432-0756
DOI:10.1051/0004-6361:20078891