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The authors acknowledge financial support from the I+D 2015 project AYA2015-65887-P (MINECO/FEDER). J.G.N also acknowledges financial support from the Spanish MINECO for a “Ramon y Cajal” fellowship (RYC-2013-13256). AL acknowledges partial support by PRIN MIUR 2015 ‘Cosmology and Fundamental Physics: illuminating the Dark Universe with Euclid’, PRIN INAF 2014 ‘Probing the AGN/galaxy co-evolution through ultra-deep and ultra-high-resolution radio surveys’, and the RADIOFOREGROUNDS grant (COMPET-05-2015, agreement number 687312) of the European Union Horizon 2020 research and innovation programme. LD, RJI and SJM acknowledge support from the ERC Advanced Grant COSMICISM, and LD and SJM also acknowledge support from the ERC Consolidator Grant, CosmicDust. MN received funding from the European Union’s Horizon2020 research and innovation programme under the Marie Sk lodowska-Curie grant agreement No 707601.