And with that, Step 7: Final Correction has commenced...
"After applying the Field of View correction, the key thing left to address is the removal of any small, residual positioning errors in the primary mirror segments. We measure and make corrections using the Fine Phasing process (Step 5). We will do a final check of the image quality across each of the science instruments; once this is verified, the wavefront sensing and controls process will be complete.
As we go through the seven steps, we may find that we need to iterate earlier steps as well. The process is flexible and modular to allow for iteration. After roughly three months of aligning the telescope, we will be ready to proceed to commissioning the instruments."