  Gravity models given by higher-order scalar curvature corrections are
believed to bear important consequences. The Einstein-Bel-Robinson gravity,
with quartic curvature modification, motivated Sajadi et al to explore static
spherically symmetric black hole solutions with perturbative methods. In this
paper, inspired by their work, we investigate AdS black hole shadows in EBR
gravity. Moreover, we demonstrate how the gravity parameter alters the energy
emission rate. Finally, we handle the same problem in the presence of plasma,
since the black holes are thought to be surrounded by a medium that changes the
geodesic of photons.
