Impact of disintegration on the dispersion angle of different arriving nuclei resulting from the disintegration of 300 EeV ⁵⁶Fe nuclei over a distance of 50 Mpc. Top: Distributions of mean squared deflection angles for different secondaries with similar mass and charge to that of ¹²C. Bottom: The angular distributions of the same products in galactic coordinates are compared to the distribution for the parent ⁵⁶Fe disregarding disintegration. The star represents the position of the source in the sky and the circular lines denote the 95% confidence limit.