Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS)

A. Durkalec; O. Le Fevre; A. Pollo; S. De La Torre; P. Cassata; B. Garilli; V. Le Brun; B. C. Lemaux; D. Maccagni; L. Pentericci; L. A.M. Tasca; R. Thomas; E. Vanzella; G. Zamorani; E. Zucca; R. Amorin; S. Bardelli; L. P. Cassara; M. Castellano; A. Cimatti; O. Cucciati; A. Fontana; M. Giavalisco; A. Grazian; N. P. Hathi; O. Ilbert; S. Paltani; B. Ribeiro; D. Schaerer; M. Scodeggio; V. Sommariva; M. Talia; L. Tresse; D. Vergani; P. Capak; S. Charlot; T. Contini; J. G. Cuby; J. Dunlop; S. Fotopoulou; A. Koekemoer; C. Lopez-Sanjuan; Y. Mellier; J. Pforr; M. Salvato; N. Scoville; Y. Taniguchi; P. W. Wang

Journal ArticleOPEN ACCESS

Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS)

Astronomy and Astrophysics (2015) 583

DOI: 10.1051/0004-6361/201425343

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Abstract

We investigate the evolution of galaxy clustering for galaxies in the redshift range 2.0

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APA

Durkalec, A., Le Fevre, O., Pollo, A., De La Torre, S., Cassata, P., Garilli, B., … Wang, P. W. (2015). Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS). Astronomy and Astrophysics, 583. https://doi.org/10.1051/0004-6361/201425343

Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS)

Abstract

Author supplied keywords

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