An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array

@article{Miettinen2017AnAS,
  title={An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array},
  author={Oskari Miettinen and Mladen Novak and Vernesa Smolvci'c and Ivan Delvecchio and M Aravena and Drew Brisbin and Alexander Karim and Eric J. Murphy and Eva Schinnerer and Marcus W. Albrecht and Herv'e Aussel and F. de Bertoldi and Peter Capak and Caitlin M. Casey and Francesca Maria Civano and Christopher C Hayward and Noelia Herrera Ruiz and Olivier Ilbert and Chunyan Jiang and Clotilde Laigle and Olivier Le F{\`e}vre and Benjamin Magnelli and Stefano Marchesi and H. J. Mccracken and Enno Middelberg and Alejandra M. Munoz Arancibia and Felipe Navarrete and Nelson D. Padilla and Dominik A. Riechers and Mara Salvato and Kimberly S. Scott and Kartik Sheth and Lidia A. M. Tasca and M Bondi and Gianni Zamorani},
  journal={Astronomy and Astrophysics},
  year={2017},
  volume={602},
  pages={1-31}
}
  • Oskari Miettinen, Mladen Novak, +32 authors Gianni Zamorani
  • Published 2017
  • Physics
  • Astronomy and Astrophysics
  • Context. The observed spatial scale of the radio continuum emission from star-forming galaxies can be used to investigate the spatial extent of active star formation, constrain the importance of cosmic-ray transport, and examine the effects of galaxy interactions. Aims. We determine the radio size distribution of a large sample of 152 submillimetre galaxies (SMGs) in the COSMOS field that were pre-selected at 1.1 mm, and later detected with the Atacama Large Millimetre/submillimetre Array… CONTINUE READING

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