Add in the option to better match distributions to observed post-gravity model. This could potentially be in the form of a triply constrained furness on the final run (i.e. when cost-function factors have been determined, on the final furness constrain to match distributions as well as to match target rows and columns).
Add in the option to better match distributions to observed post-gravity model. This could potentially be in the form of a triply constrained furness on the final run (i.e. when cost-function factors have been determined, on the final furness constrain to match distributions as well as to match target rows and columns).