The purpose of this document is to provide a final pre-launch report on the analysis of data collected for the calibration of the AXAF CCD Imaging Spectrometer (ACIS). The goal of the calibration is to provide an accurate measurement of the performance of the ACIS/HRMA instrument. Through calculation of the effects of finite source distance and gravitationaly loading on the HRMA mirror assembly it will be possible to predict the in-orbit performance of the ACIS/HRMA instrument. This will allow precise evaluation of astrophysical X-ray source models and their errors.