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