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nIFTy galaxy cluster simulations – IV. Quantifying the influence of baryons on halo properties by Cui, Weiguang, Power, Chris, Knebe, Alexander, Kay, Scott T., Sembolini, Federico, Elahi, Pascal J., Yepes, Gustavo, Pearce, Frazer, Cunnama, Daniel, Beck, Alexander M., Vecchia, Claudio Dalla, Davé, Romeel, February, Sean, Huang, Shuiyao, Hobbs, Alex, Katz, Neal, McCarthy, Ian G., Murante, Giuseppe, Perret, Valentin, Puchwein, Ewald, Read, Justin I., Saro, Alexandro, Teyssier, Romain, Thacker, Robert J.

“…The variation with respect to the median is much larger in the FP runs with different baryonic physics prescriptions than in the NR runs with different hydrodynamics solvers.…”
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