Kinetic energy in the GRB 1790817A jet during the afterglow phase. The solid red line shows the posterior distribution constructed by fitting a structured jet afterglow model to the multi-wavelength afterglow and VLBI centroid motion by Ghirlanda et al. (2019). Black dots with error bars represent the estimates presented in several other papers, all based on afterglow fitting. All estimates essentially agree within the uncertainties.