At the ILC, the luminosity-weighted average polarization at the IP needs to
be determined at the permille-level. In order to reach this goal, the combined
information from the polarimeter and the collision data is required. In this
study, a unified approach will be presented, which for the first time combines
the cross section measurements with the expected constraints from the
polarimeters. Hereby, the statistical and systematical uncertainties are taken
into account, including their correlations. This study shows that a fast spin
flip frequency is required because it easily reduces the systematic
uncertainty, while a non-perfect helicity reversal can be compensated for
within the unified approach. The final goal is to provide a realistic
estimation of the luminosity-weighted average polarization at the IP to be used
in the physic analyses.Comment: 8 pages, conference proceedings LCWS 2016 Morioka Japa