“…The use of GW polarization modes to test GR was first proposed in 1973 [160,159]. The sensitivity of resonant and interferometric detectors, as well as Doppler-tracking and pulsar-timing measurements, to the extra modes was considered in several studies [343,227,412,461,292,300,324,280,331,15,118,89,225]. In the most general setting, the problem of disentangling the modes has eight unknowns -the time series for the six polarizations, plus two direction angles that affect the projection of the modes on the detector -but only six observables, corresponding to the R 0i0j components.…”