2017
DOI: 10.1017/s1743921318000042 View full text |Buy / Rent full text
|
|

Abstract: 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 galaxies. We constrain the radio SED of a complete sample of highly star-forming galaxies (SF R > 100 M / yr) based on the VLA-COSMOS 1.4 GHz Joint and 3 GHz Large Project catalogs. We reduce archival GMRT 325 MHz and 610… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance
0
0
0
0
0
0
0
0

Publication Types

Select...

Relationship

0
0

Authors

Journals