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

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

doi:10.1051/0004-6361/201425343

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

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Salvato, M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Durkalec, A., Le Fèvre, O., Pollo, A., de la Torre, S., Cassata, P., Garilli, B., et al. (2015). Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS). Astronomy & Astrophysics, 583: A128, pp. 1-19. doi:10.1051/0004-6361/201425343.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0029-593C-0

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