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tokens: ACKNOWLEDGEMENTS The authors are grateful to the anonymous referee for the useful comments on the manuscript. The Hydrangea simulations were in part performed on the German federal maximum performance computer ‘Hazel Hen’ at the maximum performance computing centre Stuttgart (HLRS), under project GCS-HYDA/ID44067 financed through the large-scale project ‘Hydrangea’ of the Gauss Centre for Supercomputing. Further simulations were performed at the Max Planck Computing and Data Facility in Garching, Germany. This project received funding from the EU Horizon 2020 research and innovation programme under Marie Skłodowska-Curie grant agreement 747645 (ClusterGal). This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility. DiRAC is part of the National E-Infrastructure. This equipment was funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grants ST/H008519/1 and ST/K00087X/1, STFC DiRAC Operations grant ST/K003267/1, and Durham University. This work has furthermore benefitted from the use of Py-SPHViewer (Benitez-Llambay 2015). STK and DJB acknowledge support from STFC through grant ST/L000768/1. RAC is a Royal Society University Research Fellow. CDV acknowledges financial support from the Spanish Ministry of Economy and Competitiveness (MINECO) through grants AYA2014-58308 and RYC-2015-1807.