Notes. The absolute value of the scalar-product between the orientation vectors of the quadrupole and the octopole are provided in the fifth column. For an isotropic universe, this is uniformly distributed on the interval [0,1]. The last column gives the probability for such an alignment (or stronger) to occur, as determined from the FFP6 simulations. Results computed after correction for the kinematic quadrupole (KQ) are denoted by “KQ corrected”. In practice, we multiply the usual expression for the angular dependence of the KQ (see Kamionkowski & Knox 2003) in the Rayleigh-Jeans regime by factors that account for both its frequency dependence and the relative contributions of the different Planck frequencies to the component separated maps. For NILC, SEVEM, and SMICA these factors are 1.7, 1.5, and 1.7, respectively.