  In this paper, we theoretically investigate the deflection of light produced
by a topologically charged Holonomy corrected Schwarzschild black hole. The
study is carried out both in the weak field limit and in the strong field
limit. We analytically deduced the expansions for light deflection in the two
limits and, from them, we determined the observables in order to provide
elements so that observational tools are able to identify these solutions. We
model possible gravitational scenarios in order to verify the possible
gravitational characteristics of the solution.
