  Rapid-turn slow-roll inflationary trajectories have been shown to be an
attractor in two-field models, provided the turn rate is near constant and
larger than the slow-roll parameters. These trajectories can produce primordial
spectra consistent with current observations on CMB scales. We present the
generalized consistency condition for sustained rapid-turn inflationary
trajectory with two fields, arbitrary field-space metric and potential valid
for any value of the turn rate. This has to be supplemented by a second
condition to ensure slow roll evolution. Both conditions together constitute a
tool to identify inflationary trajectories with arbitrary values of the turning
rate without having to solve the equations of motion. We present a Python
package for the numerical identification of regions in field-space and
parameter space that allow for rapid-turn trajectories.
