Formally, the cross section for producing a heavy evaporation residue, σ EVR , in a complete fusion reaction is given as σ EVR (E) = πh 2 2µE ∞ =0 (2 + 1)T (E,)P CN (E,)W sur (E,) (1) where E is the center of mass energy. P CN is the fusion probability and W sur is the probability that the compound nucleus will decay by emitting particles rather than fissioning. The first term represents the capture cross section. Notice that all terms depend on and the cross section depends on the product of these terms, which are not separable. When W sur is zero or a small number due to low fission barriers at high angular momenta, the capture and fusion terms will be limited. For a series of ∼ 287 reactions leading to heavy evaporation residues with Z CN ≤ 110, we point out the implications of this fact for capture cross sections for heavy element formation reactions. From a comparison of calculated and measured evaporation residue cross sections we deduce values of the fusion probability, P CN , for some of these reactions.