The VIMOS Public Extragalactic Redshift Survey (VIPERS) An unbiased estimate of the growth rate of structure at ⟨z⟩=0.85 using the clustering of luminous blue galaxies

被引:35
|
作者
Mohammad, F. G. [1 ,2 ,3 ,4 ]
Granett, B. R. [1 ,2 ,4 ]
Guzzo, L. [1 ,2 ,4 ]
Bel, J. [1 ,2 ,5 ]
Branchini, E. [6 ,7 ,8 ]
de la Torre, S. [9 ]
Moscardini, L. [10 ,11 ,12 ]
Peacock, J. A. [13 ]
Bolzonella, M. [12 ]
Garilli, B. [14 ]
Scodeggio, M. [14 ]
Abbas, U. [15 ]
Adami, C. [9 ]
Bottini, D. [14 ]
Cappi, A. [12 ,16 ]
Cucciati, O. [10 ,12 ]
Davidzon, I. [9 ,12 ]
Franzetti, P. [14 ]
Fritz, A. [14 ]
Iovino, A. [1 ,2 ]
Krywult, J. [17 ]
Le Brun, V. [9 ]
Le Fevre, O. [9 ]
Maccagni, D. [10 ,14 ]
Malek, K. [9 ,18 ]
Marulli, F. [10 ,11 ,12 ]
Polletta, M. [19 ,20 ]
Pollo, A. [21 ]
Tasca, L. A. M. [9 ]
Tojeiro, R. [22 ]
Vergani, D. [23 ]
Zanichelli, A. [24 ]
Arnouts, S. [9 ,25 ]
Coupon, J. [26 ]
De Lucia, G. [27 ]
Ilbert, O. [9 ]
Moutard, T. [9 ,28 ]
机构
[1] INAF Osservatorio Astronomico Brera, Via Brera 28, I-20122 Milan, Italy
[2] Via E Bianchi 46, I-23807 Merate, Italy
[3] Univ Insubria, Dipartimento Sci & Alta Tecnol, Via Valleggio 11, I-22100 Como, Italy
[4] Univ Milan, Via G Celoria 16, I-20133 Milan, Italy
[5] Univ Toulon & Var, Aix Marseille Univ, CNRS, CPT, F-13288 Marseille, France
[6] Univ Rome, Dipartimento Matemat & Fis, Via Vasca Navale 84, I-00146 Rome, Italy
[7] INFN, Sez Roma Tre, Via Vasca Navale 84, I-00146 Rome, Italy
[8] INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, RM, Italy
[9] Aix Marseille Univ, CNRS, LAM, F-13388 Marseille, France
[10] Alma Mater Studiorum Univ, Dipartimento Fis & Astron, Via Gobetti 93-2, I-40129 Bologna, Italy
[11] INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
[12] INAF Osservatorio Astron Bologna, Via Gobetti 93-3, I-40129 Bologna, Italy
[13] Univ Edinburgh, Royal Observ, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
[14] INAF Ist Astrofis Spaziale & Fis Cosm Milano, Via Bassini 15, I-20133 Milan, Italy
[15] INAF Osservatorio Astrofis Torino, I-10025 Pino Torinese, Italy
[16] Univ Nice Sophia Antipolis, CNRS, Lab Lagrange, UMR 7293,Observ Cote Azur, F-06300 Nice, France
[17] Jan Kochanowski Univ, Inst Phys, Ul Swietokrzyska 15, PL-25406 Kielce, Poland
[18] Natl Ctr Nucl Res, Ul Hoza 69, PL-00681 Warsaw, Poland
[19] Aix Marseille Univ, 58 Bd Charles Livon, F-13284 Marseille 7, France
[20] IRAP, Av 9 Colonel Roche,BP 44346, F-31028 Toulouse 4, France
[21] Jagiellonian Univ, Astron Observ, Orla 171, PL-30001 Krakow, Poland
[22] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Scotland
[23] INAF Ist Astrofis Spaziale & Fis Cosm Bologna, Via Gobetti 101, I-40129 Bologna, Italy
[24] INAF Ist Radioastron, Via Gobetti 101, I-40129 Bologna, Italy
[25] Canada France Hawaii Telescope, 65-1238 Mamalahoa Highway, Kamuela, HI 96743 USA
[26] Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland
[27] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy
[28] St Marys Univ, Dept Astron & Phys, 923 Robie St, Halifax, NS B3H 3C3, Canada
基金
欧洲研究理事会;
关键词
cosmology: observations; large-scale structure of Universe; galaxies: high-redshift; galaxies: statistics; SPACE DISTORTIONS; COLOR DEPENDENCE; PECULIAR VELOCITIES; SYSTEMATIC-ERRORS; POWER-SPECTRUM; REAL-SPACE; SCALE; MODEL; HALOES; EVOLUTION;
D O I
10.1051/0004-6361/201731685
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We used the VIMOS Public Extragalactic Redshift Survey (VIPERS) final data release (PDR-2) to investigate the performance of colour-selected populations of galaxies as tracers of linear large-scale motions. We empirically selected volume-limited samples of blue and red galaxies as to minimise the systematic error on the estimate of the growth rate of structure f sigma(8) from the anisotropy of the two-point correlation function. To this end, rather than rigidly splitting the sample into two colour classes we defined the red or blue fractional contribution of each object through a weight based on the (U-V) colour distribution. Using mock surveys that are designed to reproduce the observed properties of VIPERS galaxies, we find the systematic error in recovering the fiducial value of f sigma(8) to be minimised when using a volume-limited sample of luminous blue galaxies. We modelled non-linear corrections via the Scoccimarro extension of the Kaiser model (with updated fitting formulae for the velocity power spectra), finding systematic errors on f sigma(8) of below 1-2%, using scales as small as 5 h(-1) Mpc. We interpret this result as indicating that selection of luminous blue galaxies maximises the fraction that are central objects in their dark matter haloes; this in turn minimises the contribution to the measured xi(r(p), pi) from the 1-halo term, which is dominated by non-linear motions. The gain is inferior if one uses the full magnitude-limited sample of blue objects, consistent with the presence of a significant fraction of blue, fainter satellites dominated by non-streaming, orbital velocities. We measured a value of f sigma(8) = 0.45 +/- 0.11 over the single redshift range 0.6 <= z <= 1.0, corresponding to an effective redshift for the blue galaxies < z > = 0.85. Including in the likelihood the potential extra information contained in the blue-red galaxy cross-correlation function does not lead to an appreciable improvement in the error bars, while it increases the systematic error.
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页数:20
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