Star formation rates as a function of stellar masses of the galaxy members in the spectroscopically confirmed structure G237+42.50 (ss1+ss2) from Polletta et al. (2021) (black stars). A grey circle indicates the AGN members. The SFR and stellar masses of the galaxies from the closest simulated case (for ss1 and ss2) are shown as blue crosses, and a cyan circle is over-plotted on those that are considered AGN. The main sequence at z = 2.17, as formulated by Speagle et al. (2014), is shown as a solid red line, and the main sequence divided by a factor of three as a dotted red line.