The VIMOS VLT Deep Survey

C. Marinoni; L. Guzzo; A. Cappi; O. Le Fèvre; A. Mazure; B. Meneux; A. Pollo; A. Iovino; H. J. McCracken; R. Scaramella; S. De La Torre; J. M. Virey; D. Bottini; B. Garilli; V. Le Brun; D. MacCagni; J. P. Picat; M. Scodeggio; L. Tresse; G. Vettolani; A. Zanichelli; C. Adami; S. Arnouts; S. Bardelli; M. Bolzonella; S. Charlot; P. Ciliegi; T. Contini; S. Foucaud; P. Franzetti; I. Gavignaud; O. Ilbert; F. Lamareille; B. Marano; G. Mathez; R. Merighi; S. Paltani; R. Pellò; L. Pozzetti; M. Radovich; D. Vergani; G. Zamorani; E. Zucca; U. Aabbas; M. Bondi; A. Bongiorno; J. Brinchmann; A. Buzzi; O. Cucciati; L. De Ravel; L. Gregorini; Y. Mellier; P. Merluzzi; E. Perez-Montero; P. Taxil; S. Temporin; C. J. Walcher

doi:10.1051/0004-6361:20078891

The VIMOS VLT Deep Survey

C. Marinoni, L. Guzzo, A. Cappi, O. Le Fèvre, A. Mazure, B. Meneux, A. Pollo, A. Iovino, H. J. McCracken, R. Scaramella, S. De La Torre, J. M. Virey, D. Bottini, B. Garilli, V. Le Brun, D. MacCagni, J. P. Picat, M. Scodeggio, L. Tresse, G. VettolaniA. Zanichelli, C. Adami, S. Arnouts, S. Bardelli, M. Bolzonella, S. Charlot, P. Ciliegi, T. Contini, S. Foucaud, P. Franzetti, I. Gavignaud, O. Ilbert, F. Lamareille, B. Marano, G. Mathez, R. Merighi, S. Paltani, R. Pellò, L. Pozzetti, M. Radovich, D. Vergani, G. Zamorani, E. Zucca, U. Aabbas, M. Bondi, A. Bongiorno, J. Brinchmann, A. Buzzi, O. Cucciati, L. De Ravel, L. Gregorini, Y. Mellier, P. Merluzzi, E. Perez-Montero, P. Taxil, S. Temporin, C. J. Walcher

Facultad Ciencias Exactas

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

13 Citas (Scopus)

Resumen

We have reconstructed the three-dimensional density fluctuation maps to 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 . We apply a self-consistent reconstruction scheme which includes a complete non-linear description of galaxy biasing and which has been thoroughly tested on realistic mock samples. We find that the variance and skewness of the galaxy distribution evolve over this redshift interval in a way that is remarkably consistent with predictions of first- and second-order perturbation theory. This finding confirms the standard gravitational instability paradigm over nearly 9 Gyr of cosmic time and demonstrates the importance of accounting for the non-linear component of galaxy biasing to consistently reproduce the higher-order moments of the galaxy distribution and their evolution.

Idioma original	Inglés
Páginas (desde-hasta)	7-17
Número de páginas	11
Publicación	Astronomy and Astrophysics
Volumen	487
N.º	1
DOI	https://doi.org/10.1051/0004-6361:20078891
Estado	Publicada - ago. 2008

Áreas temáticas de ASJC Scopus

Astronomía y astrofísica
Ciencias planetarias y espacial

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10.1051/0004-6361:20078891

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Marinoni, C., Guzzo, L., Cappi, A., Le Fèvre, O., Mazure, A., Meneux, B., Pollo, A., Iovino, A., McCracken, H. J., Scaramella, R., De La Torre, S., Virey, J. M., Bottini, D., Garilli, B., Le Brun, V., MacCagni, D., Picat, J. P., Scodeggio, M., Tresse, L., ... Walcher, C. J. (2008). The VIMOS VLT Deep Survey. Astronomy and Astrophysics, 487(1), 7-17. https://doi.org/10.1051/0004-6361:20078891

@article{77d6c8d62a04497e934cb47c46a8ca67,

title = "The VIMOS VLT Deep Survey",

abstract = "We have reconstructed the three-dimensional density fluctuation maps to 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 . We apply a self-consistent reconstruction scheme which includes a complete non-linear description of galaxy biasing and which has been thoroughly tested on realistic mock samples. We find that the variance and skewness of the galaxy distribution evolve over this redshift interval in a way that is remarkably consistent with predictions of first- and second-order perturbation theory. This finding confirms the standard gravitational instability paradigm over nearly 9 Gyr of cosmic time and demonstrates the importance of accounting for the non-linear component of galaxy biasing to consistently reproduce the higher-order moments of the galaxy distribution and their evolution.",

keywords = "Cosmology: large-scale structure of Universe, Cosmology: theory, Galaxies: high-redshift, Galaxies: statistics, Galaxy: evolution",

author = "C. Marinoni and L. Guzzo and A. Cappi and {Le F{\`e}vre}, O. and A. Mazure and B. Meneux and A. Pollo and A. Iovino and McCracken, {H. J.} and R. Scaramella and {De La Torre}, S. and Virey, {J. M.} and D. Bottini and B. Garilli and {Le Brun}, V. and D. MacCagni and Picat, {J. P.} and M. Scodeggio and L. Tresse and G. Vettolani and A. Zanichelli and C. Adami and S. Arnouts and S. Bardelli and M. Bolzonella and S. Charlot and P. Ciliegi and T. Contini and S. Foucaud and P. Franzetti and I. Gavignaud and O. Ilbert and F. Lamareille and B. Marano and G. Mathez and R. Merighi and S. Paltani and R. Pell{\`o} and L. Pozzetti and M. Radovich and D. Vergani and G. Zamorani and E. Zucca and U. Aabbas and M. Bondi and A. Bongiorno and J. Brinchmann and A. Buzzi and O. Cucciati and {De Ravel}, L. and L. Gregorini and Y. Mellier and P. Merluzzi and E. Perez-Montero and P. Taxil and S. Temporin and Walcher, {C. J.}",

year = "2008",

month = aug,

doi = "10.1051/0004-6361:20078891",

language = "English",

volume = "487",

pages = "7--17",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "1",

}

Marinoni, C, Guzzo, L, Cappi, A, Le Fèvre, O, Mazure, A, Meneux, B, Pollo, A, Iovino, A, McCracken, HJ, Scaramella, R, De La Torre, S, Virey, JM, Bottini, D, Garilli, B, Le Brun, V, MacCagni, D, Picat, JP, Scodeggio, M, Tresse, L, Vettolani, G, Zanichelli, A, Adami, C, Arnouts, S, Bardelli, S, Bolzonella, M, Charlot, S, Ciliegi, P, Contini, T, Foucaud, S, Franzetti, P, Gavignaud, I, Ilbert, O, Lamareille, F, Marano, B, Mathez, G, Merighi, R, Paltani, S, Pellò, R, Pozzetti, L, Radovich, M, Vergani, D, Zamorani, G, Zucca, E, Aabbas, U, Bondi, M, Bongiorno, A, Brinchmann, J, Buzzi, A, Cucciati, O, De Ravel, L, Gregorini, L, Mellier, Y, Merluzzi, P, Perez-Montero, E, Taxil, P, Temporin, S & Walcher, CJ 2008, 'The VIMOS VLT Deep Survey', Astronomy and Astrophysics, vol. 487, n.º 1, pp. 7-17. https://doi.org/10.1051/0004-6361:20078891

TY - JOUR

T1 - The VIMOS VLT Deep Survey

AU - Marinoni, C.

AU - Guzzo, L.

AU - Cappi, A.

AU - Le Fèvre, O.

AU - Mazure, A.

AU - Meneux, B.

AU - Pollo, A.

AU - Iovino, A.

AU - McCracken, H. J.

AU - Scaramella, R.

AU - De La Torre, S.

AU - Virey, J. M.

AU - Bottini, D.

AU - Garilli, B.

AU - Le Brun, V.

AU - MacCagni, D.

AU - Picat, J. P.

AU - Scodeggio, M.

AU - Tresse, L.

AU - Vettolani, G.

AU - Zanichelli, A.

AU - Adami, C.

AU - Arnouts, S.

AU - Bardelli, S.

AU - Bolzonella, M.

AU - Charlot, S.

AU - Ciliegi, P.

AU - Contini, T.

AU - Foucaud, S.

AU - Franzetti, P.

AU - Gavignaud, I.

AU - Ilbert, O.

AU - Lamareille, F.

AU - Marano, B.

AU - Mathez, G.

AU - Merighi, R.

AU - Paltani, S.

AU - Pellò, R.

AU - Pozzetti, L.

AU - Radovich, M.

AU - Vergani, D.

AU - Zamorani, G.

AU - Zucca, E.

AU - Aabbas, U.

AU - Bondi, M.

AU - Bongiorno, A.

AU - Brinchmann, J.

AU - Buzzi, A.

AU - Cucciati, O.

AU - De Ravel, L.

AU - Gregorini, L.

AU - Mellier, Y.

AU - Merluzzi, P.

AU - Perez-Montero, E.

AU - Taxil, P.

AU - Temporin, S.

AU - Walcher, C. J.

PY - 2008/8

Y1 - 2008/8

N2 - We have reconstructed the three-dimensional density fluctuation maps to 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 . We apply a self-consistent reconstruction scheme which includes a complete non-linear description of galaxy biasing and which has been thoroughly tested on realistic mock samples. We find that the variance and skewness of the galaxy distribution evolve over this redshift interval in a way that is remarkably consistent with predictions of first- and second-order perturbation theory. This finding confirms the standard gravitational instability paradigm over nearly 9 Gyr of cosmic time and demonstrates the importance of accounting for the non-linear component of galaxy biasing to consistently reproduce the higher-order moments of the galaxy distribution and their evolution.

AB - We have reconstructed the three-dimensional density fluctuation maps to 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 . We apply a self-consistent reconstruction scheme which includes a complete non-linear description of galaxy biasing and which has been thoroughly tested on realistic mock samples. We find that the variance and skewness of the galaxy distribution evolve over this redshift interval in a way that is remarkably consistent with predictions of first- and second-order perturbation theory. This finding confirms the standard gravitational instability paradigm over nearly 9 Gyr of cosmic time and demonstrates the importance of accounting for the non-linear component of galaxy biasing to consistently reproduce the higher-order moments of the galaxy distribution and their evolution.

KW - Cosmology: large-scale structure of Universe

KW - Cosmology: theory

KW - Galaxies: high-redshift

KW - Galaxies: statistics

KW - Galaxy: evolution

UR - http://www.scopus.com/inward/record.url?scp=48249130888&partnerID=8YFLogxK

U2 - 10.1051/0004-6361:20078891

DO - 10.1051/0004-6361:20078891

M3 - Article

AN - SCOPUS:48249130888

SN - 0004-6361

VL - 487

SP - 7

EP - 17

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 1

ER -

The VIMOS VLT Deep Survey

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