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

A. Katsianis, V Gonzalez, D. Barrientos +9

There is a severe tension between the observed star formation rate (SFR) - stellar mass (${\mathrm{M}}_{\star }$) relations reported by different authors at $z=1-4$. In addition, the o…