The prevalence of core emission in faint radio galaxies in the SKA Simulated Skies
Empirical simulations based on extrapolations from well-established low-frequency (<5 GHz) surveys fail to accurately model the faint, high frequency (>10 GHz) source population; they underpredict the number of observed sources by a factor of 2 below S18GHz = 10 mJy and fail to reprodu...
| Main Authors: | , , , , |
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| Format: | Journal article |
| Published: |
Oxford University Press
2017
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