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We describe how to apply the transport method to compute inflationaryobservables in a broad range of multiple-field models. The method is efficientand encompasses scenarios with curved field-space metrics, violations ofslow-roll conditions and turns of the trajectory in field space. It can be usedfor an arbitrary mass spectrum, including massive modes and models withquasi-single-field dynamics. In this note we focus on practical issues. It isaccompanied by a Mathematica code which can be used to explore suitable models,or as a basis for further development.

Computing observables in curved multifield models of inflation - A guide (with code) to the transport method