The VMR profiles of SO₂ and daughter species for the same atmospheres given as examples in Figure 2 for T-1 c and e. The format is the same as for Figure 2. For T-1 c and e, we show one example profile for every stable composition for each of the two planets. Only the mixed CO–CO₂ and O₂–H₂O–CO₂ compositions had nonnegligible abundances of SO₃, SO, and H₂SO₄, which is why no mixing ratio profiles are seen for these species in the other compositional cases.