Using determinant Quantum Monte Carlo, we compare three methods of evaluating the DC Hall coefficient RH of the Hubbard model: the direct measurement of the off-diagonal current-current correlator χxy in a system coupled to a finite magnetic field (FF), χ FF xy ; the three-current linear response to an infinitesimal field as measured in the zero-field (ZF) Hubbard Hamiltonian, χ ZF xy ; and the leading order recurrent expansionH in terms of thermodynamic susceptibilities. The two quantities χ FF xy and χ ZF xy can be compared directly in imaginary time. Proxies for RH constructed from the three-current correlator χ ZF xy can be determined under different simplifying assumptions and compared with R (0) H . We find these different quantities to be consistent with one another, validating previous conclusions about the close correspondence between Fermi surface topology and the sign of RH , even for strongly correlated systems. These various quantities also provide a useful set of numerical tools for testing theoretical predictions about the full behavior of the Hall conductivity for strong correlations.