Shapley supercluster survey: galaxy evolution from filaments to cluster cores

Merluzzi, P.; Busarello, G.; Haines, C. P.; Mercurio, A.; Okabe, N.; Pimbblet, K. J.; Dopita, M. A.; Grado, A.; Limatola, L.; Bourdin, H.; Mazzotta, P.; Capaccioli, M.; Napolitano, N. R.; Schipani, P.

Shapley supercluster survey: galaxy evolution from filaments to cluster cores

Date

2015-01

Authors

Merluzzi, P.

Busarello, G.

Haines, C. P.

Mercurio, A.

Okabe, N.

Pimbblet, K. J.

Dopita, M. A.

Grado, A.

Limatola, L.

Bourdin, H.

Publisher

Oxford University Press

Abstract

We present an overview of a multiwavelength survey of the Shapley Supercluster (SSC; z ~ 0.05) covering a contiguous area of 260 h70 -2 Mpc2 including the supercluster core. The project main aim is to quantify the influence of cluster-scale mass assembly