Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field

We investigate how the shape of the galaxy two-point correlation function as measured in the zCOSMOS survey depends on local environment, quantified in terms of the density contrast on scales of 5 Mpc/h. We show that the flat shape previously observed at redshifts between z=0.6 and z=1 can be explai...

Täydet tiedot

Bibliografiset tiedot
Päätekijät:	Torre, S, Guzzo, L, Kovac, K, Porciani, C, Abbas, U, Meneux, B, Carollo, C, Contini, T, Kneib, J, Fevre, O, Lilly, S, Mainieri, V, Renzini, A, Sanders, D, Scodeggio, M, Scoville, N, Zamorani, G, Bardelli, S, Bolzonella, M, Bongiorno, A, Caputi, K, Coppa, G, Cucciati, O, Ravel, L, Franzetti, P
Aineistotyyppi:	Journal article
Kieli:	English
Julkaistu:	2010

Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field

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