Unravelling lifecycles & physics of radio-loud AGN in the SKA era
Radio-loud AGN (> 10 22 W Hz-1 at 1.4 GHz) will be the dominant bright source population detected with the SKA. The high resolution that the SKA will provide even in wide-area surveys will mean that, for the first time sensitive, multi-frequency total intensity and polarisation imaging of large s...
| Main Authors: | , , , , , |
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| Other Authors: | |
| Format: | Conference Paper |
| Published: |
Proceedings of Science
2014
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| Online Access: | http://pos.sissa.it/archive/conferences/215/173/AASKA14_173.pdf http://hdl.handle.net/20.500.11937/16644 |