Relative calibration coefficients found when calibrating on the orbital dipole (constant gain, light blue, with bogopix in red) and using CMB anisotropies (see Sect. 6.2, in green), with respect to the solar dipole gains, used to build the HFI maps. As ADC non-linearities are not corrected for, calibration systematics depend on the amplitude on the signal used to check for them. The amplitudes of such effects are within the systematic uncertainties quoted in Table 6.