1. 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. Issue 4 (20th January 2020) Authors: Katsianis, A; Gonzalez, V; Barrientos, D; Yang, X; Lagos, C D P; Schaye, J; Camps, P; Trčka, A; Baes, M; Stalevski, M; Blanc, G A; Theuns, T Journal: Monthly notices of the Royal Astronomical Society Issue: Volume 492:Issue 4(2020) Page Start: 5592 Record Type: Journal Article View Content: Available online (eLD content is only available in our Reading Rooms) ↗