Final results of shear measurement for CSST with our FORKLENS approach. The first panel displays the shear residuals obtained after calibration using NNs, while the second panel shows the shear residuals after applying galaxy weighting. Both panels consist of measurements from the same set of 20 million galaxies. Each data point represents 100 000 galaxy and PSF pairs with varying properties, but sharing the same shear. Shape noise cancellation was not employed.