ner_tags: O O O O O O O O O O O O O O O O B-Person O B-Person I-Person O O O O O B-Person I-Person I-Person I-Person O B-Person I-Person O O O O O O O O O O O O O O O O O B-Telescope O O O O B-Telescope O O O O B-Organization I-Organization I-Organization I-Organization I-Organization O O B-Organization I-Organization I-Organization I-Organization I-Organization O O O O O O B-Grant I-Grant I-Grant I-Grant I-Grant B-Grant O O O O O O O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization O B-Location O O O B-Organization I-Organization I-Organization I-Organization I-Organization O B-Location O O O O B-Proposal I-Proposal I-Proposal I-Proposal I-Proposal I-Proposal I-Proposal O O O O O O O O B-Organization I-Organization I-Organization B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization B-Organization O O O B-Grant O B-Software I-Software I-Software O O O O O O O B-Survey I-Survey I-Survey B-Survey O O O O O O O B-Observatory O O O B-Observatory I-Observatory O B-Observatory I-Observatory O O O B-Grant O B-Software I-Software I-Software O O O O O O O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization B-Organization O O B-Organization I-Organization I-Organization I-Organization O O O O O O O O O B-Citation I-Citation I-Citation I-Citation O O O O B-Survey O O B-URL O
tokens: We are grateful to an anonymous referee for helpful comments and suggestions that improved this work. JR thanks Lister Staveley-Smith for useful comments. We thank Claudia del P. Lagos and Han-Seek Kim for providing their model predictions used in Fig. 11 . We also thank the staff of the GMRT for their assistance. The GMRT is operated by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. This research was funded by an Australian Indian Strategic Research Fund (AISRF) grant. This fund was jointly administered by the Department of Innovation, Industry, Science and Research in Australia and by the Department of Science and Technology in India. The project title was ‘Gas in Galaxies in the Distant Past’. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. The G10/COSMOS 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 catalogue can be found in (Davies et al. 2015 ) or on the G10 website at http://ict.icrar.org/cutout/G10/ .