Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-28T01:23:26.977Z Has data issue: false hasContentIssue false
  • English
  • Français

The Scientific Potential of LOFAR for Time Domain Astronomy

Published online by Cambridge University Press:  20 April 2012

Rob Fender
Rob Fender*
Affiliation:
School of Physics & Astronomy, University of Southampton, SO17 1BJ, UK For TKSP member list see: www.transientskp.org/team.shtml email: [email protected]
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.

LOFAR is a ground-breaking low-frequency radio telescope that is currently nearing completion across northern Europe. As a software telescope with no moving parts, enormous fields of view and multi-beaming, it has fantastic potential for the exploration of the time-variable universe. In this brief paper I outline LOFAR's capabilities, our plans to use it for a range of transient searches, and some crude estimated rates of transient detections.

Keywords

accretionstars:binariesstars:pulsarsstars:supernovae:generalISM: jets and outflowsradio continuum: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S285: New Horizons in Time-Domain Astronomy , September 2011 , pp. 11 - 16
Copyright
Copyright © International Astronomical Union 2012

References

Bell, M. E. 2011, PhD thesis, University of SouthamptonGoogle Scholar
Bower, G. C., et al. , 2007, ApJ, 6, 346CrossRefGoogle Scholar
Frail, D. A., et al. , 2011, ApJ, submittedGoogle Scholar
Seaman, R., et al. , 2011, IVOA Recommendation, arXiv:1110.0523Google Scholar
Stappers, B. W., Hessels, J. W. T., Alexov, A., et al. , 2011, A&A, 530, 80Google Scholar