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I extract new limits on the coefficient of the effective operator generated by tree-level graviton exchange in large extra dimensions from $pp \rightarrow jjM_T > 6.82.6 fb^{-1}$ of integrated luminosity) and TeV (ATLAS after ). I also compare such limits to the ones obtained using the full graviton amplitude, and discuss the impact of additional constrains arising from other datasets, such as Mono-Jet.

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