Variations of fluxes and rotation diagrams depending on stellar parameters. Top left: same as Figure 7, but showing line fluxes for models with enhanced FUV and X-ray luminosities: 10 times (green) and 100 times (blue) the fiducial L_X, and 4 times (yellow) and 40 times (pink) the fiducial L_FUV. The lower-mass run (M_* = 0.4 M_⊙ with 10 times the fiducial L_X) is also included (light green). All fluxes are computed with i = 90° and without disk obscuration. Note that the spatial integration regions and distance differ between our model and the observations (see the caption of Figure 7). Top right: same as the top-left panel, but with reduced fluxes due to disk obscuration. Bottom left: rotation diagram, same as Figure 9, but using the fluxes from the top-left panel. Bottom right: Rotation diagram using the fluxes with disk obscuration from the top-right panel.