Persistent URL of this record https://hdl.handle.net/1887/3134418
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- 2001.06025
- Accepted Manuscript
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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
- 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
- Volume
- 492
- Issue
- 4
- Pages
- 5592 - 5606