The infrared-radio correlation of star-forming galaxies is strongly M$_{\star}$-dependent but nearly redshift-invariant since z$\sim$4 (2020)

First Author: Delvecchio I
Attributed to:  Astrophysics at Oxford 2016-2019 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2010.05510

Publication URI: https://arxiv.org/abs/2010.05510

Type: Other