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tokens: Acknowledgements GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programmes including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel -ATLAS, GMRT, and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/ . Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 179.A-2004. The G10-COSMOS redshift catalogue, photometric catalogue, and cutout tool uses data acquired as part of the Cosmic Evolution Survey (COSMOS) project and spectra from observations made with ESO Telescopes at the La Silla or Paranal Observatories under programme ID 175.A-0839. The G10-COSMOS cutout tool is hosted and maintained by funding from the International Centre for Radio Astronomy Research (ICRAR) at the University of Western Australia. Full details of the data, observation, and catalogues can be found in Davies et al. ( 2015 ) and Andrews et al. ( 2017a ), or on the G10-COSMOS website: cutout.icrar.org/G10/dataRelease.php This work is based on observations by the 3D-HST Treasury Program (GO 12177 and 12328) with the NASA/ESA HST , which is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS5-26555. This work was supported by resources provided by the Pawsey Supercomputing Centre with funding from the Australian Government and the Government of Western Australia. SKA is supported by an Australian Postgraduate Award. LJD and SJM acknowledge support from European Research Council (ERC) in the form of Advanced Investigator grant COSMICISM and Consolidator grant Cosmic Dust.