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We identify shocked gas in simulated galaxy clusters extracted from theMareNostrum Universe simulation (Gottloeber et al. 2006) assuming that shockwaves are regions of electron acceleration. We perform flux number countswithin the framework of the non-thermal emission model developed by Hoeft etal. (2008). Results are presented at two different observing frequencies, i.e.1.4 GHz and 120 MHz, posing interesting constraints for LOFAR and upcomingradio telescopes.

Radio relics in the MareNostrum Universe