Average radio spectral energy distribution of highly star-forming galaxies

Autor: Tisanić, K., Smolčić, V., Delhaize, J., Novak, M., Intema, H.T., Delvecchio, I., Schinnerer, E., Zamorani, G., Jelić V., Hulst T. van der

Publikováno v: Proceedings of the International Astronomical Union
Proceedings of the International Astronomical Union, 191-194. IAU
ISSUE=S333;STARTPAGE=191;ENDPAGE=194;TITLE=Proceedings of the International Astronomical Union

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

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eab442b0c45df7aab87f9b2434488d99
https://hdl.handle.net/21.11116/0000-0005-CAAC-6