The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of highly star-forming galaxies
We construct the average radio spectral energy distribution (SED) of highly star-forming galaxies (HSFGs) up to z ~ 4. Infrared and radio luminosities are bound by a tight correlation that is defined by the so-called q parameter. This infrared-radio correlation provides the basis for the use of radi...
| Main Authors: | , , , , , , , , , |
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| Format: | Journal Article |
| Published: |
EDP Sciences
2019
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| Online Access: | http://hdl.handle.net/20.500.11937/73666 |