Origin of cosmic chemical abundances
Umberto Maio, Edoardo Tescari
Monthly Notices of the Royal Astronomical Society | OXFORD UNIV PRESS | Published : 2015
Related Projects (2)
Awarded by Marie Curie Fellowship by the European Union Seventh Framework Programme (FP7)
Awarded by Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)
We thank the anonymous referee for detailed and constructive comments which helped us extend and improve significantly the original manuscript. We acknowledge useful discussions with A. Arino-i-Prats, S. Borgani, J. Cooke, R. Cooke, S. Cristiani, G. De Lucia, K. Dolag, F. Matteucci, P. Molaro, M. Viel, F. A. Villaescusa Navarro and F. Vincenzo. UM was supported through a Marie Curie Fellowship by the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement no. 267251. ET is supported by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO) through project number CE110001020. This research was undertaken with the assistance of resources from the National Computational Infrastructure (NCI),<SUP>14</SUP> which is supported by the Australian Government. We would like to thank Volker Springel for making available to us the non-public version of the GADGET-3 code. For the simulations we used the raijin, vayu and xe clusters at the NCI National Facility. For the post-processing, we also used the edward High Performance Computing (HPC) cluster at the University of Melbourne.<SUP>15</SUP> Mass functions have been computed by means of the online calculator http://hmf.icrar.org by Murray, Power & Robotham (2013). We acknowledge the NASA Astrophysics Data System and the JSTOR archives for their bibliographic tools.