The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1

B. Mcneux; L. Guzzo; B. Gariili; O. Le Fevre; A. Polio; J. Blaizot; G. De Lucia; M. Boizoncila; F. Larnarcillc; L. Pozzetti; A. Cappi; A. Iovino; C. Marinoni; H. J. Mccrackcn; S. De La Torre; D. Bottini; V. Le Brun; D. Maccagnl; J. P. Picat; R. Scaramella; M. Scodeggio; L. Tressc; G. Vcttolani; U. Abbas; S. Arnouts; S. Bardclli; A. Bongiomo; S. Chariot; P. Ciliegi; T. Contini; O. Cucciatl; S. Foucaud; P. Ftanzetti; I. Gavignaud; O. Ilbert; B. Marano; A. Manure; R. Mcrighi; S. Paltani; R. Pello; M. Radovich; D. Vcrgani; G. Zamorani; E. Zucca

The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1

B. Mcneux, L. Guzzo, B. Gariili, O. Le Fevre, A. Polio, J. Blaizot, G. De Lucia, M. Boizoncila, F. Larnarcillc, L. Pozzetti, A. Cappi, A. Iovino, C. Marinoni, H. J. Mccrackcn, S. De La Torre, D. Bottini, V. Le Brun, D. Maccagnl, J. P. Picat, R. ScaramellaM. Scodeggio, L. Tressc, G. Vcttolani, U. Abbas, S. Arnouts, S. Bardclli, A. Bongiomo, S. Chariot, P. Ciliegi, T. Contini, O. Cucciatl, S. Foucaud, P. Ftanzetti, I. Gavignaud, O. Ilbert, B. Marano, A. Manure, R. Mcrighi, S. Paltani, R. Pello, M. Radovich, D. Vcrgani, G. Zamorani, E. Zucca

Exact Sciences School

Research output: Contribution to conference › Paper › peer-review

Abstract

We have investigated the dependence of galaxy clustering on their stellar mass at z~l, using the data from the VIMOS-VLT Deep Survey (WDS). We have measured the projected two- point correlation function of galaxies, tnP{rp) for a set of stellar mass selected samples at an effective redshift < z >= 0.85. We have control aud quantify all effects on galaxy clustering due to the incompleteness of our low mass samples. We find that more massive galaxies are more clustered When compared to similar results at ∗ ~ 0.1 in the SDSS: we observed no evolution of the projected correlation function for massive galaxies. These objects present a stronger linear bias at z ~ 1 with rcspcct to low mass galaxies. As expcctcd, massive objects at high redshift arc found in the highest pics of the dark matter density field.

Original language	English
Pages	223-226
Number of pages	4
Publication status	Published - 1 Jan 2018
Event	2008 43rd Rencontres de Moriond on Cosmology - La Thuile Val d'Aosta, Italy Duration: 15 Mar 2008 → 22 Mar 2008

Conference

Conference	2008 43rd Rencontres de Moriond on Cosmology
Country/Territory	Italy
City	La Thuile Val d'Aosta
Period	15/03/08 → 22/03/08

ASJC Scopus subject areas

Astronomy and Astrophysics

Cite this

Mcneux, B., Guzzo, L., Gariili, B., Le Fevre, O., Polio, A., Blaizot, J., De Lucia, G., Boizoncila, M., Larnarcillc, F., Pozzetti, L., Cappi, A., Iovino, A., Marinoni, C., Mccrackcn, H. J., De La Torre, S., Bottini, D., Le Brun, V., Maccagnl, D., Picat, J. P., ... Zucca, E. (2018). The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1. 223-226. Paper presented at 2008 43rd Rencontres de Moriond on Cosmology, La Thuile Val d'Aosta, Italy.

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title = "The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1",

abstract = "We have investigated the dependence of galaxy clustering on their stellar mass at z~l, using the data from the VIMOS-VLT Deep Survey (WDS). We have measured the projected two- point correlation function of galaxies, tnP{rp) for a set of stellar mass selected samples at an effective redshift < z >= 0.85. We have control aud quantify all effects on galaxy clustering due to the incompleteness of our low mass samples. We find that more massive galaxies are more clustered When compared to similar results at ∗ ~ 0.1 in the SDSS: we observed no evolution of the projected correlation function for massive galaxies. These objects present a stronger linear bias at z ~ 1 with rcspcct to low mass galaxies. As expcctcd, massive objects at high redshift arc found in the highest pics of the dark matter density field.",

author = "B. Mcneux and L. Guzzo and B. Gariili and {Le Fevre}, O. and A. Polio and J. Blaizot and {De Lucia}, G. and M. Boizoncila and F. Larnarcillc and L. Pozzetti and A. Cappi and A. Iovino and C. Marinoni and Mccrackcn, {H. J.} and {De La Torre}, S. and D. Bottini and {Le Brun}, V. and D. Maccagnl and Picat, {J. P.} and R. Scaramella and M. Scodeggio and L. Tressc and G. Vcttolani and U. Abbas and S. Arnouts and S. Bardclli and A. Bongiomo and S. Chariot and P. Ciliegi and T. Contini and O. Cucciatl and S. Foucaud and P. Ftanzetti and I. Gavignaud and O. Ilbert and B. Marano and A. Manure and R. Mcrighi and S. Paltani and R. Pello and M. Radovich and D. Vcrgani and G. Zamorani and E. Zucca",

note = "Funding Information: BM thanks the organisers of the conference for the financial support. LG gratefully acknowledges the hospitality of MPE, MPA and ESO. Publisher Copyright: {\textcopyright} 2018 Proceedings - 43rd Rencontres de Moriond on Cosmology. All rights reserved.; 2008 43rd Rencontres de Moriond on Cosmology ; Conference date: 15-03-2008 Through 22-03-2008",

year = "2018",

month = jan,

day = "1",

language = "English",

pages = "223--226",

}

Mcneux, B, Guzzo, L, Gariili, B, Le Fevre, O, Polio, A, Blaizot, J, De Lucia, G, Boizoncila, M, Larnarcillc, F, Pozzetti, L, Cappi, A, Iovino, A, Marinoni, C, Mccrackcn, HJ, De La Torre, S, Bottini, D, Le Brun, V, Maccagnl, D, Picat, JP, Scaramella, R, Scodeggio, M, Tressc, L, Vcttolani, G, Abbas, U, Arnouts, S, Bardclli, S, Bongiomo, A, Chariot, S, Ciliegi, P, Contini, T, Cucciatl, O, Foucaud, S, Ftanzetti, P, Gavignaud, I, Ilbert, O, Marano, B, Manure, A, Mcrighi, R, Paltani, S, Pello, R, Radovich, M, Vcrgani, D, Zamorani, G & Zucca, E 2018, 'The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1', Paper presented at 2008 43rd Rencontres de Moriond on Cosmology, La Thuile Val d'Aosta, Italy, 15/03/08 - 22/03/08 pp. 223-226.

TY - CONF

T1 - The vimos-vlt deep survey

T2 - 2008 43rd Rencontres de Moriond on Cosmology

AU - Mcneux, B.

AU - Guzzo, L.

AU - Gariili, B.

AU - Le Fevre, O.

AU - Polio, A.

AU - Blaizot, J.

AU - De Lucia, G.

AU - Boizoncila, M.

AU - Larnarcillc, F.

AU - Pozzetti, L.

AU - Cappi, A.

AU - Iovino, A.

AU - Marinoni, C.

AU - Mccrackcn, H. J.

AU - De La Torre, S.

AU - Bottini, D.

AU - Le Brun, V.

AU - Maccagnl, D.

AU - Picat, J. P.

AU - Scaramella, R.

AU - Scodeggio, M.

AU - Tressc, L.

AU - Vcttolani, G.

AU - Abbas, U.

AU - Arnouts, S.

AU - Bardclli, S.

AU - Bongiomo, A.

AU - Chariot, S.

AU - Ciliegi, P.

AU - Contini, T.

AU - Cucciatl, O.

AU - Foucaud, S.

AU - Ftanzetti, P.

AU - Gavignaud, I.

AU - Ilbert, O.

AU - Marano, B.

AU - Manure, A.

AU - Mcrighi, R.

AU - Paltani, S.

AU - Pello, R.

AU - Radovich, M.

AU - Vcrgani, D.

AU - Zamorani, G.

AU - Zucca, E.

N1 - Funding Information: BM thanks the organisers of the conference for the financial support. LG gratefully acknowledges the hospitality of MPE, MPA and ESO. Publisher Copyright: © 2018 Proceedings - 43rd Rencontres de Moriond on Cosmology. All rights reserved.

PY - 2018/1/1

Y1 - 2018/1/1

N2 - We have investigated the dependence of galaxy clustering on their stellar mass at z~l, using the data from the VIMOS-VLT Deep Survey (WDS). We have measured the projected two- point correlation function of galaxies, tnP{rp) for a set of stellar mass selected samples at an effective redshift < z >= 0.85. We have control aud quantify all effects on galaxy clustering due to the incompleteness of our low mass samples. We find that more massive galaxies are more clustered When compared to similar results at ∗ ~ 0.1 in the SDSS: we observed no evolution of the projected correlation function for massive galaxies. These objects present a stronger linear bias at z ~ 1 with rcspcct to low mass galaxies. As expcctcd, massive objects at high redshift arc found in the highest pics of the dark matter density field.

AB - We have investigated the dependence of galaxy clustering on their stellar mass at z~l, using the data from the VIMOS-VLT Deep Survey (WDS). We have measured the projected two- point correlation function of galaxies, tnP{rp) for a set of stellar mass selected samples at an effective redshift < z >= 0.85. We have control aud quantify all effects on galaxy clustering due to the incompleteness of our low mass samples. We find that more massive galaxies are more clustered When compared to similar results at ∗ ~ 0.1 in the SDSS: we observed no evolution of the projected correlation function for massive galaxies. These objects present a stronger linear bias at z ~ 1 with rcspcct to low mass galaxies. As expcctcd, massive objects at high redshift arc found in the highest pics of the dark matter density field.

UR - http://www.scopus.com/inward/record.url?scp=85067243583&partnerID=8YFLogxK

M3 - Paper

AN - SCOPUS:85067243583

SP - 223

EP - 226

Y2 - 15 March 2008 through 22 March 2008

ER -

The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1

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ASJC Scopus subject areas

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