Acknowlegements

NuGrid acknowledges support from NSF grants PHY 02-16783 and PHY 08-22648 (Joint Institute for Nuclear Astrophysics, JINA), NSF grant PHY-1430152 (JINA Center for the Evolution of the Elements), EU MIRG-CT-2006-046520 and STFC (through the University of Hull’s Consolidated Grant ST/R000840/1), ChETEC COST Action (CA16117) supported by COST (European Cooperation in Science and Technology), and from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 101008324 (ChETEC-INFRA). The continued work on codes and in disseminating data is made possible through funding from STFC (RH, UK), an NSERC Discovery grant (FH, Canada) and support from SNF (MP, Switzerland). NuGrid computations are performed at the high-performance computer KHAOS at EPSAM Institute at Keele University (UK) as well as CFI (Canada) funded computing resources at the Department of Physics and Astronomy at the University of Victoria and through Computing Time Resource Allocation through the Compute Canada WestGrid consortium. We also acknowledge support by the STFC DiRAC High Performance Computing Facilities, and ongoing resource allocations on the University of Hulls High Performance Computing Facility VIPER. The collaboration uses services of the Canadian Advanced Network for Astronomy Research (CANFAR) which in turn is supported by CANARIE, Compute Canada, University of Victoria, the National Research Council of Canada, and the Canadian Space Agency. RH acknowledges support from the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan and funding from the European Research Council under the European Union’s Seventh Framework Programme (FP/2007-2013) / ERC Grant Agreement n. 306901. TP acknowledges support from the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)-Project No. 279384907-SFB 1245, and the State of Hesse within the Research Cluster ELEMENTS (Project ID 500/10.006).