Observed distance from core (top) and flux density (bottom) for every one of the identified component as a function of time, together with a linear weighted fit to knot distance and logarithmic fit to flux. The fit to the flux is done taking into account only the points after the peak of emission of each component. This was done for all components except B7, which due to its low flux, did not have enough points after the peak with low enough uncertainty to perform a fit.