“…With reference to the gravity model (2), nodal attractions, P i (or P j ), are computed endogenously with exogenous spatial interactions, G ij , and spatial impedance, F ðd ij Þ, hence a reverse-fitting of the gravity model. This paper simplifies the general reverse-fitting algebraic method developed in Shen (1999Shen ( , 2002. The algebraic simplification is novel in that it substantially reduces the size of the spatial interaction matrix required by the algebraic method for estimating good-fit nodal attractions.…”