Final masses of protoplanetary embryos in simulations of Model I where t_start = 0.5 Myr and the size of the rocky pebbles is Rocky_peb = 0.1 cm for different pebble fluxes S_peb. Each panel shows the outcome of ten different simulations with slightly different initial conditions. Each final planetary object is represented by a colored dot where the color represents its final ice mass fraction. Planetary objects belonging to the same simulation are connected by lines. The integrated pebble fluxes are ~ 39 M_⊕, ~ 78 M_⊕, ~ 194 M_⊕, and ~ 485 M_⊕ for S_peb = 0.2,  0.4,  1,  and 2.5, respectively. The efficiency of pebble accretion (fraction of integrated pebble flux used to build planets) is about 17, 25, 32, and 30% for S_peb = 0.2, 0.4, 1, and 2.5, respectively.