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tokens: Acknowledgments The SILCC project details are available at http://www.astro.uni-koeln.de/silcc . All simulations have been performed on the Odin and Hydra clusters hosted by the Max Planck Computing Data Facility ( http://www.mpcdf.mpg.de/ ). We thank M. Anderson, C. Federrath, J. Mackey, M. M. Mac Low, E. Pellegrini, and X. Shi for useful discussions and Leroy etal. ( 2008 ) and Ekstrm etal. ( 2012 ) for making their data publicly available. AG, SW, TN, PG, SCOG, RSK, and TP acknowledge the Deutsche Forschungsgemeinschaft (DFG) for funding through the SPP 1573 The Physics of the Interstellar Medium. SW acknowledges funding by the Bonn-Cologne-Graduate School, by SFB 956 The conditions and impact of star formation, and from the European Research Council under the European Communitys Framework Programme FP8 via the ERC Starting Grant RADFEEDBACK (project number 679852). TN acknowledges support by the DFG cluster of excellence Origin and Structure of the Universe. RW acknowledges support by the Czech Science Foundation project 15-06012S and by the institutional project RVO: 67985815. RSK and SCOG acknowledge support from the DFG via SFB 881 The Milky Way System (sub-projects B1, B2, and B8). RSK acknowledges support from the European Research Council under the European Communitys Seventh Framework Programme (FP7/2007-2013) via the ERC Advanced Grant STARLIGHT (project number 339177). The software used in this work was in part developed by the DOE NNSA-ASC OASCR Flash Center at the University of Chicago. We thank C. Karch for the program package fy and M. Turk and the yt community for the yt project (Turk etal. 2011 ).