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A general formalism to include experimental reaction cross sections intocalculations of stellar rates is presented. It also allows to assess themaximally possible reduction of uncertainties in the stellar rates byexperiments. As an example for the application of the procedure, stellarneutron capture reactivities from KADoNiS v0.3 are revised and the remaininguncertainties shown. Many of the uncertainties in the stellar rates are largerthan those obtained experimentally. This has important consequences fors-process models and the interpretation of meteoritic data because it allowsthe rates of some reactions to vary within a larger range than previouslyassumed.

Formalism for inclusion of measured reaction cross sections in stellar  rates including uncertainties and its application to neutron capture in the  s-process