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 & 24 otros 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

Resultado de la investigación: Paper

Resumen

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.

Idioma originalEnglish
Páginas223-226
Número de páginas4
EstadoPublished - 1 ene 2018
Evento2008 43rd Rencontres de Moriond on Cosmology - La Thuile Val d'Aosta, Italy
Duración: 15 mar 200822 mar 2008

Conference

Conference2008 43rd Rencontres de Moriond on Cosmology
PaísItaly
CiudadLa Thuile Val d'Aosta
Período15/03/0822/03/08

Huella dactilar

stellar mass
galaxies
dark matter
arcs

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Citar esto

Mcneux, B., Guzzo, L., Gariili, B., Le Fevre, O., Polio, A., Blaizot, J., ... Zucca, E. (2018). The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1. 223-226. Papel presentado en 2008 43rd Rencontres de Moriond on Cosmology, La Thuile Val d'Aosta, Italy.
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. ; 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. / The vimos-vlt deep survey : the dependence of clustering on galaxy stellar mass at 2~1. Papel presentado en 2008 43rd Rencontres de Moriond on Cosmology, La Thuile Val d'Aosta, Italy.4 p.
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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",
year = "2018",
month = "1",
day = "1",
language = "English",
pages = "223--226",
note = "2008 43rd Rencontres de Moriond on Cosmology ; Conference date: 15-03-2008 Through 22-03-2008",

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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' Papel presentado en 2008 43rd Rencontres de Moriond on Cosmology, La Thuile Val d'Aosta, Italy, 15/03/08 - 22/03/08, pp. 223-226.

The vimos-vlt deep survey : the dependence of clustering on galaxy stellar mass at 2~1. / 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.; 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. 223-226 Papel presentado en 2008 43rd Rencontres de Moriond on Cosmology, La Thuile Val d'Aosta, Italy.

Resultado de la investigación: Paper

TY - CONF

T1 - The vimos-vlt deep survey

T2 - the dependence of clustering on galaxy stellar mass at 2~1

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.

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

SP - 223

EP - 226

ER -

Mcneux B, Guzzo L, Gariili B, Le Fevre O, Polio A, Blaizot J y otros. The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1. 2018. Papel presentado en 2008 43rd Rencontres de Moriond on Cosmology, La Thuile Val d'Aosta, Italy.