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...

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Bibliographic Details
Main Authors: Tisanic, K., Smolcic, V., Delhaize, J., Novak, M., Intema, Hubertus, Delvecchio, I., Schinnerer, E., Zamorani, G., Bondi, M., Vardoulaki, E.
Format: Journal Article
Published: EDP Sciences 2019
Online Access:http://hdl.handle.net/20.500.11937/73666