VIMOS-VLT deep survey: Evolution of the large scale structure of the universe from z 2 until now

Agnieszka Pollo; Ummi Abbas; Baptiste Meneux; Luigi Guzzo; Olivier Le Fèvre; D. Bottini; B. Garilli; V. Le Brun; D. Maccagni; M. Scodeggio; L. Tresse; G. Vettolani; A. Zanichelli; C. Adami; S. Arnouts; S. Bardelli; M. Bolzonella; A. Cappi; S. Charlot; P. Ciliegi; T. Contini; S. Foucaud; P. Franzetti; I. Gavignaud; O. Ilbert; A. Iovino; F. Lamareille; H. J. McCracken; C. Marinoni; A. Mazure; R. Merighi; S. Paltani; R. Pellò; L. Pozzetti; D. Vergani; G. Zamorani; E. Zucca

VIMOS-VLT deep survey: Evolution of the large scale structure of the universe from z 2 until now

Agnieszka Pollo, Ummi Abbas, Baptiste Meneux, Luigi Guzzo, Olivier Le Fèvre, D. Bottini, B. Garilli, V. Le Brun, D. Maccagni, M. Scodeggio, L. Tresse, G. Vettolani, A. Zanichelli, C. Adami, S. Arnouts, S. Bardelli, M. Bolzonella, A. Cappi, S. Charlot, P. CiliegiT. Contini, S. Foucaud, P. Franzetti, I. Gavignaud, O. Ilbert, A. Iovino, F. Lamareille, H. J. McCracken, C. Marinoni, A. Mazure, R. Merighi, S. Paltani, R. Pellò, L. Pozzetti, D. Vergani, G. Zamorani, E. Zucca

Facultad Ciencias Exactas

Producción científica: Contribución a una revista › Artículo de la conferencia › revisión exhaustiva

Resumen

We discuss the evolution of clustering of galaxies back to z 2. For that purpose we use the VIMOS-VLT Deep Survey (VVDS) data. We analyze the evolution of the projected two-point correlation function for the global galaxy population and for particular galaxy classes, with different intrinsic luminosities, spectral types, colors and other properties. For the brightest galaxies (with L>L^*), for instance, the shape of the correlation function deviated from the power-law much more strongly at z 1 than it is observed now. This finding can be interpreted e.g. in the framework of Halo Occupation Distribution models (HODs) and implies a significant change in the way luminous galaxies traced dark-matter halos at z 1 with respect to now. Our observations represent an important constraint for models trying to reproduce the evolution of galaxy clustering.

Idioma original	Inglés
Publicación	Proceedings of Science
Estado	Publicada - 1 dic. 2009
Evento	European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009 - Krakow, Polonia Duración: 16 jul. 2009 → 22 jul. 2009

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Pollo, A., Abbas, U., Meneux, B., Guzzo, L., Le Fèvre, O., Bottini, D., Garilli, B., Le Brun, V., Maccagni, D., Scodeggio, M., Tresse, L., Vettolani, G., Zanichelli, A., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., ... Zucca, E. (2009). VIMOS-VLT deep survey: Evolution of the large scale structure of the universe from z 2 until now. Proceedings of Science.

@article{f1296d304bb244e7a8a2766f42779bb0,

title = "VIMOS-VLT deep survey: Evolution of the large scale structure of the universe from z 2 until now",

abstract = "We discuss the evolution of clustering of galaxies back to z 2. For that purpose we use the VIMOS-VLT Deep Survey (VVDS) data. We analyze the evolution of the projected two-point correlation function for the global galaxy population and for particular galaxy classes, with different intrinsic luminosities, spectral types, colors and other properties. For the brightest galaxies (with L>L*), for instance, the shape of the correlation function deviated from the power-law much more strongly at z 1 than it is observed now. This finding can be interpreted e.g. in the framework of Halo Occupation Distribution models (HODs) and implies a significant change in the way luminous galaxies traced dark-matter halos at z 1 with respect to now. Our observations represent an important constraint for models trying to reproduce the evolution of galaxy clustering.",

author = "Agnieszka Pollo and Ummi Abbas and Baptiste Meneux and Luigi Guzzo and {Le F{\`e}vre}, Olivier and D. Bottini and B. Garilli and {Le Brun}, V. and D. Maccagni 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 A. Cappi and S. Charlot and P. Ciliegi and T. Contini and S. Foucaud and P. Franzetti and I. Gavignaud and O. Ilbert and A. Iovino and F. Lamareille and McCracken, {H. J.} and C. Marinoni and A. Mazure and R. Merighi and S. Paltani and R. Pell{\`o} and L. Pozzetti and D. Vergani and G. Zamorani and E. Zucca",

year = "2009",

month = dec,

day = "1",

language = "English",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

note = "European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009 ; Conference date: 16-07-2009 Through 22-07-2009",

}

Pollo, A, Abbas, U, Meneux, B, Guzzo, L, Le Fèvre, O, Bottini, D, Garilli, B, Le Brun, V, Maccagni, D, Scodeggio, M, Tresse, L, Vettolani, G, Zanichelli, A, Adami, C, Arnouts, S, Bardelli, S, Bolzonella, M, Cappi, A, Charlot, S, Ciliegi, P, Contini, T, Foucaud, S, Franzetti, P, Gavignaud, I, Ilbert, O, Iovino, A, Lamareille, F, McCracken, HJ, Marinoni, C, Mazure, A, Merighi, R, Paltani, S, Pellò, R, Pozzetti, L, Vergani, D, Zamorani, G & Zucca, E 2009, 'VIMOS-VLT deep survey: Evolution of the large scale structure of the universe from z 2 until now', Proceedings of Science.

TY - JOUR

T1 - VIMOS-VLT deep survey

T2 - European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009

AU - Pollo, Agnieszka

AU - Abbas, Ummi

AU - Meneux, Baptiste

AU - Guzzo, Luigi

AU - Le Fèvre, Olivier

AU - Bottini, D.

AU - Garilli, B.

AU - Le Brun, V.

AU - Maccagni, D.

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 - Cappi, A.

AU - Charlot, S.

AU - Ciliegi, P.

AU - Contini, T.

AU - Foucaud, S.

AU - Franzetti, P.

AU - Gavignaud, I.

AU - Ilbert, O.

AU - Iovino, A.

AU - Lamareille, F.

AU - McCracken, H. J.

AU - Marinoni, C.

AU - Mazure, A.

AU - Merighi, R.

AU - Paltani, S.

AU - Pellò, R.

AU - Pozzetti, L.

AU - Vergani, D.

AU - Zamorani, G.

AU - Zucca, E.

PY - 2009/12/1

Y1 - 2009/12/1

N2 - We discuss the evolution of clustering of galaxies back to z 2. For that purpose we use the VIMOS-VLT Deep Survey (VVDS) data. We analyze the evolution of the projected two-point correlation function for the global galaxy population and for particular galaxy classes, with different intrinsic luminosities, spectral types, colors and other properties. For the brightest galaxies (with L>L*), for instance, the shape of the correlation function deviated from the power-law much more strongly at z 1 than it is observed now. This finding can be interpreted e.g. in the framework of Halo Occupation Distribution models (HODs) and implies a significant change in the way luminous galaxies traced dark-matter halos at z 1 with respect to now. Our observations represent an important constraint for models trying to reproduce the evolution of galaxy clustering.

AB - We discuss the evolution of clustering of galaxies back to z 2. For that purpose we use the VIMOS-VLT Deep Survey (VVDS) data. We analyze the evolution of the projected two-point correlation function for the global galaxy population and for particular galaxy classes, with different intrinsic luminosities, spectral types, colors and other properties. For the brightest galaxies (with L>L*), for instance, the shape of the correlation function deviated from the power-law much more strongly at z 1 than it is observed now. This finding can be interpreted e.g. in the framework of Halo Occupation Distribution models (HODs) and implies a significant change in the way luminous galaxies traced dark-matter halos at z 1 with respect to now. Our observations represent an important constraint for models trying to reproduce the evolution of galaxy clustering.

UR - http://www.scopus.com/inward/record.url?scp=84891907615&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:84891907615

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

Y2 - 16 July 2009 through 22 July 2009

ER -

VIMOS-VLT deep survey: Evolution of the large scale structure of the universe from z 2 until now

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