Average radio spectral energy distribution of highly star-forming galaxies

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Average radio spectral energy distribution of highly star-forming galaxies

The infrared-radio correlation (IRRC) offers a way to assess star formation from radio emission. Multiple studies found the IRRC to decrease with increasing redshift. This may in part be due to the lack of knowledge about the possible radio spectral energy distributions (SEDs) of star-forming galaxi...

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Bibliographic Details
Main Authors:	Tisanic, K., Smolcic, V., Delhaize, J., Novak, M., Intema, Hubertus, Delvecchio, I., Schinnerer, E., Zamorani, G.
Format:	Journal Article
Published:	2017
Online Access:	http://hdl.handle.net/20.500.11937/74483

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