Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-14T06:37:11.979Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio Surveys: an Overview

Published online by Cambridge University Press:  05 March 2015

Raffaella Morganti
Raffaella Morganti*
Affiliation:
Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, The Netherlands email: morganti@astron.nl Kapteyn Astronomical Institute, University of Groningen, Postbus 800, 9700 AV Groningen, The Netherlands
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Radio astronomy has provided important surveys that have made possible key (and sometimes serendipitous) discoveries. I will briefly mention some of the past continuum and line (HI) radio surveys as well as new, on-going surveys and surveys planned for the near future. This new generation of large radio surveys is bringing extra challenges in terms of data handling but also great new possibilities thanks to the wider range of data products that they will provide.

Keywords

surveysradio continuum: galaxiesradio lines: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 667 - 668
Copyright
Copyright © International Astronomical Union 2015 

References

Barnes, D. G., et al. 2001, MNRAS, 322, 486CrossRefGoogle Scholar
Giovanelli, R., et al. 2005 AJ 130, 2598CrossRefGoogle Scholar
Heald, G., et al. 2011, JApA, 32, 589Google Scholar
Johnston, S., et al. 2008, ExA, 22, 151Google Scholar
Kellermann, K., et al. 2009, PoS 99, 5Google Scholar
Norris, R. P., et al. 2012, arXiv, arXiv:1210.7521Google Scholar
Oosterloo, T., et al. 2009, “SKA 2009”, PoS 132, 70Google Scholar
Röttgering, H., et al. 2011, JApA, 32, 557Google Scholar