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Hi there!
Currently, in PHOEBE 2.4.21, spots added to a star always rotate with the stellar surface according to syncpar and to changelog. This works as expected for synchronous stars; however, for stars with syncpar > 1 spots are automatically asynchronous in the orbital frame, which prevents modelling hotspots near L1 as stationary in the orbital frame. According to the API and source code, there is no documented way to fix a spot in the orbital frame (or is it?). Is there a method to achieve this, or could future updates include support for spots stationary in orbital phase?
Cheers!
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