The comparison of the calculated Doppler broadening of the and lines with the result of the proposed experiment will allow us to perform a fine tuning of the Coulomb and deceleration rates. The data on the kinetic energy distribution obtained with the nToF method will also be used for this goal. By transferring this information into the part of the cascade calculations we are confident that the current uncertainties in the calculated energy distributions of the atom at the instant of the X-ray transitions will be reduced to the level allowing to predict the Doppler broadening correction to the X-ray lines profile with an error of better than 1% in the hadronic width.