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
Author(s):
Katsianis, A.; Gonzalez, V.; Barrientos, D.; Yang, X.; Lagos, C.D.P.; Schaye, J. (0000-0002-0668-5560); Camps, P.; Trčka, A.; Baes, M.; Stalevski, M.; Blanc, G.A.; Theuns, T.
Published
2020
Publication type
Article / Letter to editor
Date issued
2020-01-20
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2020), Vol. 492, no. 4, p. 5592-5606
