Maybe the pulsations of these stars, (across the broader set of known Cepheids), have never been as accurate as they'd like to think.
As telescopes are get more precise, you'd kind of expect that the variations in pulsations, would become more noticeable. (After all, all observations contain uncertainties. These are also a moving target).
Still, chalk another one up for the stellar evolution theory in its never-ending 'tug-o-war' with the stellar pulsation theory.
Last time we looked at this, the report was that stellar pulsation had produced highly accurate estimates in the mass predictions for an eclipsing binary cepheid.
The period vs luminosity relationship has really only been known for about 100 years, and the ionised Helium mechanism was only proposed in 1953.
Is this really sufficient time for us to expect that all known Cepheid pulsations should be as expected ?
Cheers