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The VIMOS-VLT Deep Survey: evolution in the halo occupation number since z∼ 1★: VVDS: evolution in the HON over z = 0-1.3

U. Abbas,S. De La Torre,O. Le Fèvre,L. Guzzo,C. Marinoni,B. Meneux,A. Pollo,G. Zamorani,D. Bottini,B. Garilli,V. Le Brun, D. Maccagni,R. Scaramella,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,B. Marano,A. Mazure,R. Merighi, S. Paltani,R. Pellò,L. Pozzetti,M. Radovich,D. Vergani,E. Zucca,M. Bondi,A. Bongiorno,J. Brinchmann, O. Cucciati,L. De Ravel,L. Gregorini,E. Perez-Montero, Y. Mellier,P. Merluzzi

Monthly Notices of the Royal Astronomical Society（2010）

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摘要
We model the evolution of the mean galaxy occupation of dark matter haloes over the range 0.1 < z < 1.3, using the data from the VIMOS-VLT Deep Survey. The galaxy projected correlation function wp(rp) was computed for a set of luminosity-limited subsamples and fits to its shape were obtained using two variants of halo occupation distribution (HOD) models. These provide us with a set of best-fittin...
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methods: statistical,surveys,galaxies: high-redshift,large-scale structure of Universe
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