Same as Fig. 7 except that we now use Model III, where the embryos are initially spread from 0.3 to 2.0 AU. The integrated pebble fluxes are ~ 194 M_⊕, ~ 485 M_⊕, ~ 970 M_⊕, and ~ 1940 M_⊕ for S_peb = 1,  2.5,  5,  and 10, respectively. The efficiency of pebble accretion is about 4.3, 2.1, 1.6, and 1.4% for S_peb = 1,  2.5,  5,  and 10, respectively.Clearly, the most massive bodies in each simulation have a large water fraction.