Sorry for bringing this old post up again.
Very simple: it's infinite. That is, if there should only be one STO, we only use one STO, rather than fudging it with a high eta2.
If this is true, it should mean that C1 == 1, otherwise the orbital isn't normalized.
But this is not the case for the Cerda parameters.
My calculation:
Radial part of a singe STO is
R(n,C1,et1,r) = { r^(n-1) / sqrt[(2n)!] } * C1 * (2*eta1)^(n+1/2) * exp(-eta1*r)
If I integrate R(n,C1,et1,r)^2*r^2 dr from 0 to infinity I get a surprisingly simple result: it's C1^2.
Thus, the normalization condition is C1^2 == 1. Or am I wrong here?