HM and CC microlensing light curves of limb-darkened and blended source stars are plotted, but we additionally consider a close-in giant planet around each source star. Details are similar to those in Fig. 5. In each panel, the source star (blue circle), its planet (red circle), the planet orbit projected on the sky plane (green curve), and the lens trajectory (black solid line) are shown as insets in the figures. The chromatic perturbations in the V -I and B-R stellar colors by considering only the LD and BL effects (solid) and LD, BL plus a source star planet (dashed) are shown in the residual parts with black and gray curves. Their parameters are given in Table 4.