The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years

A. Pollo; U. Abbas; B. Meneux; L. Guzzo; O. Le Fèvre; A. Cappi; H. J. McCracken; A. Iovino; C. Marinoni; D. Bottini; B. Garilli; V. Le Brun; D. Maccagni; J. P. Picat; R. Scaramella; 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; B. Marano; A. Mazure; R. Merighi; S. Paltani; R. Pellò; L. Pozzetti; M. Radovich; G. Zamorani; E. Zucca; M. Bondi; A. Bongiorno; J. Brinchmann; O. Cucciati; S. De La Torre; F. Lamareille; Y. Mellier; P. Merluzzi; S. Temporin; D. Vergani; C. J. Walcher

doi:10.1393/ncb/i2008-10467-0

The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years

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

Facultad Ciencias Exactas

Producción científica: Contribución a los distintos tipos de conferencia › Artículo › revisión exhaustiva

Resumen

Using the first-epoch data from the VIMOS-VLT Deep Survey (VVDS), we investigate the evolution of the projected two-point correlation function of galaxies between z ∼ 1 and the present epoch. For the global galaxy population we do not find strong variations of clustering with redshift. However, dependence of clustering on intrinsic luminosities and stellar masses of galaxies evolves significantly during this period. We observe more close pairs for the most luminous and (less distinctly) most massive objects at z ∼ 1 as compared to what is seen locally, resulting in a non-power-law shape of their correlation function, with an upturn on small scales. This effect can be modeled within the framework of the halo occupation distribution models and leads to the conclusion that at z ∼ 1 we are possibly observing a population of luminous and not very massive satellite galaxies that occupy the most massive dark-matter halos - an effect that is not seen locally.

Idioma original	Inglés
Páginas	1203-1208
Número de páginas	6
DOI	https://doi.org/10.1393/ncb/i2008-10467-0
Estado	Publicada - 2007
Evento	A Century of Cosmology: Past, Present and Future - San Servolo, Venice, Italia Duración: 27 ago. 2007 → 31 ago. 2007

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Otros	A Century of Cosmology: Past, Present and Future
País/Territorio	Italia
Ciudad	San Servolo, Venice
Período	27/08/07 → 31/08/07

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Astronomía y astrofísica

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10.1393/ncb/i2008-10467-0

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Pollo, A., Abbas, U., Meneux, B., Guzzo, L., Le Fèvre, O., Cappi, A., McCracken, H. J., Iovino, A., Marinoni, C., Bottini, D., Garilli, B., Le Brun, V., Maccagni, D., Picat, J. P., Scaramella, R., Scodeggio, M., Tresse, L., Vettolani, G., Zanichelli, A., ... Walcher, C. J. (2007). The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years. 1203-1208. Papel presentado en A Century of Cosmology: Past, Present and Future, San Servolo, Venice, Italia. https://doi.org/10.1393/ncb/i2008-10467-0

@conference{097a0f927c3a41f9af06b2b979156b6b,

title = "The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years",

abstract = "Using the first-epoch data from the VIMOS-VLT Deep Survey (VVDS), we investigate the evolution of the projected two-point correlation function of galaxies between z ∼ 1 and the present epoch. For the global galaxy population we do not find strong variations of clustering with redshift. However, dependence of clustering on intrinsic luminosities and stellar masses of galaxies evolves significantly during this period. We observe more close pairs for the most luminous and (less distinctly) most massive objects at z ∼ 1 as compared to what is seen locally, resulting in a non-power-law shape of their correlation function, with an upturn on small scales. This effect can be modeled within the framework of the halo occupation distribution models and leads to the conclusion that at z ∼ 1 we are possibly observing a population of luminous and not very massive satellite galaxies that occupy the most massive dark-matter halos - an effect that is not seen locally.",

author = "A. Pollo and U. Abbas and B. Meneux and L. Guzzo and {Le F{\`e}vre}, O. and A. Cappi and McCracken, {H. J.} and A. Iovino and C. Marinoni and D. Bottini and B. Garilli and {Le Brun}, V. and D. Maccagni and Picat, {J. P.} and R. Scaramella 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 B. Marano and A. Mazure and R. Merighi and S. Paltani and R. Pell{\`o} and L. Pozzetti and M. Radovich and G. Zamorani and E. Zucca and M. Bondi and A. Bongiorno and J. Brinchmann and O. Cucciati and {De La Torre}, S. and F. Lamareille and Y. Mellier and P. Merluzzi and S. Temporin and D. Vergani and Walcher, {C. J.}",

year = "2007",

doi = "10.1393/ncb/i2008-10467-0",

language = "English",

pages = "1203--1208",

}

Pollo, A, Abbas, U, Meneux, B, Guzzo, L, Le Fèvre, O, Cappi, A, McCracken, HJ, Iovino, A, Marinoni, C, Bottini, D, Garilli, B, Le Brun, V, Maccagni, D, Picat, JP, Scaramella, R, 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, Marano, B, Mazure, A, Merighi, R, Paltani, S, Pellò, R, Pozzetti, L, Radovich, M, Zamorani, G, Zucca, E, Bondi, M, Bongiorno, A, Brinchmann, J, Cucciati, O, De La Torre, S, Lamareille, F, Mellier, Y, Merluzzi, P, Temporin, S, Vergani, D & Walcher, CJ 2007, 'The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years', Papel presentado en A Century of Cosmology: Past, Present and Future, San Servolo, Venice, Italia, 27/08/07 - 31/08/07 pp. 1203-1208. https://doi.org/10.1393/ncb/i2008-10467-0

The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years. / Pollo, A.; Abbas, U.; Meneux, B. et al.
2007. 1203-1208 Papel presentado en A Century of Cosmology: Past, Present and Future, San Servolo, Venice, Italia.

Producción científica: Contribución a los distintos tipos de conferencia › Artículo › revisión exhaustiva

TY - CONF

T1 - The VIMOS-VLT Deep Survey

T2 - A Century of Cosmology: Past, Present and Future

AU - Pollo, A.

AU - Abbas, U.

AU - Meneux, B.

AU - Guzzo, L.

AU - Le Fèvre, O.

AU - Cappi, A.

AU - McCracken, H. J.

AU - Iovino, A.

AU - Marinoni, C.

AU - Bottini, D.

AU - Garilli, B.

AU - Le Brun, V.

AU - Maccagni, D.

AU - Picat, J. P.

AU - Scaramella, R.

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 - Marano, B.

AU - Mazure, A.

AU - Merighi, R.

AU - Paltani, S.

AU - Pellò, R.

AU - Pozzetti, L.

AU - Radovich, M.

AU - Zamorani, G.

AU - Zucca, E.

AU - Bondi, M.

AU - Bongiorno, A.

AU - Brinchmann, J.

AU - Cucciati, O.

AU - De La Torre, S.

AU - Lamareille, F.

AU - Mellier, Y.

AU - Merluzzi, P.

AU - Temporin, S.

AU - Vergani, D.

AU - Walcher, C. J.

PY - 2007

Y1 - 2007

N2 - Using the first-epoch data from the VIMOS-VLT Deep Survey (VVDS), we investigate the evolution of the projected two-point correlation function of galaxies between z ∼ 1 and the present epoch. For the global galaxy population we do not find strong variations of clustering with redshift. However, dependence of clustering on intrinsic luminosities and stellar masses of galaxies evolves significantly during this period. We observe more close pairs for the most luminous and (less distinctly) most massive objects at z ∼ 1 as compared to what is seen locally, resulting in a non-power-law shape of their correlation function, with an upturn on small scales. This effect can be modeled within the framework of the halo occupation distribution models and leads to the conclusion that at z ∼ 1 we are possibly observing a population of luminous and not very massive satellite galaxies that occupy the most massive dark-matter halos - an effect that is not seen locally.

AB - Using the first-epoch data from the VIMOS-VLT Deep Survey (VVDS), we investigate the evolution of the projected two-point correlation function of galaxies between z ∼ 1 and the present epoch. For the global galaxy population we do not find strong variations of clustering with redshift. However, dependence of clustering on intrinsic luminosities and stellar masses of galaxies evolves significantly during this period. We observe more close pairs for the most luminous and (less distinctly) most massive objects at z ∼ 1 as compared to what is seen locally, resulting in a non-power-law shape of their correlation function, with an upturn on small scales. This effect can be modeled within the framework of the halo occupation distribution models and leads to the conclusion that at z ∼ 1 we are possibly observing a population of luminous and not very massive satellite galaxies that occupy the most massive dark-matter halos - an effect that is not seen locally.

UR - http://www.scopus.com/inward/record.url?scp=84907085565&partnerID=8YFLogxK

U2 - 10.1393/ncb/i2008-10467-0

DO - 10.1393/ncb/i2008-10467-0

M3 - Paper

AN - SCOPUS:84907085565

SP - 1203

EP - 1208

Y2 - 27 August 2007 through 31 August 2007

ER -

The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years

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