Similar to Fig. 3, but including the effect of the excess gaseous carbon caused by the reset scenario of carbon depletion. The carbon advects inward quickly, disappearing before 1 Myr. The ongoing scenario would maintain the same level of carbon excess over the lifetime of the disk. Additionally we overplot the radial evolution of the three targeted planets. The dots along each track denote thepoint at which (starting from the bottom) the planet begins accreting gas, when it has accreted 3 M_⊕ of gas, and when the planet has reached half of its final mass. The inner two planets accrete their gas primarily within the ice line, while the outer planet accretes its gas between the CO₂ and CO ice lines.