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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) A. Katsianis, V. Gonzalez, Daniela Barrientos Acevedo (UGent), X. Yang, C. D. P. Lagos, J. Schaye, Peter Camps (UGent), Ana Trčka (UGent), Maarten Baes (UGent), Marko Stalevski (UGent), G. A. Blanc, T. Theuns
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