SEDs computed for parameters given in Table 1. SEDs are time averaged. Each line corresponds to a model with a different temperature ratio in the accretion disk, (T_p/T_e)_d = 10,15 and 20, and various inclinations. The red dashed line is the “best-bet” model from Mościbrodzka et al. (2009), which assumes i ≈ 90° and T_p/T_e = 3 in the entire computational domain. The data points are the same as those used in Mościbrodzka et al. (2009). The bottom-right panel shows the sizes of the GRMHD jet model including scatter-broadening. Open symbols are Sgr A* measured sizes from Bower et al. (2006) and Doeleman et al. (2008) (1.3 mm).