Contribution to the diffuse radio background from extragalactic radio sources
We examine the brightness of the Cosmic Radio Background (CRB) by comparing the contribution from individual source counts to absolute measurements. We use a compilation of radio counts to estimate the contribution of detected sources to the CRB in several different frequency bands. Using a Monte Ca...
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Language: | English |
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University of British Columbia
2011
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Online Access: | http://hdl.handle.net/2429/37898 |
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