The high-redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: towards addressing the tension between observations and simulations (2020)

First Author: Katsianis A
Attributed to:  DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission] funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa157

Publication URI: http://dx.doi.org/10.1093/mnras/staa157

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4