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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

Katsianis, A.; Gonzalez, V.; Barrientos, D.; Yang, X.; Lagos, C.D.P.; Schaye, J.; ... ; Theuns, T. (2020)

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

Article / Letter to editor

All 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.

Date: 2020-01-20

Journal: Monthly Notices of the Royal Astronomical Society

Volume: 492

Issue: 4

Pages: 5592 - 5606

DOI: doi:10.1093/mnras/staa157

Link: https://ui.adsabs.harvard.edu/abs/2020MNRAS.492.5592K