I've here the 3rd edition, where it seems that the authors try to derive the Coulomb field of a static point charge. As to be expected from this book, it's all buried in some strange pedagogics, making the problem more complicated than it is.
The idea is simply to use the spherical symmetry of the problem. So let the point charge, ##Q##, sit at rest in the origin of a Cartesian coordinate system. We want to calculate ##\vec{E}(\vec{r})## at any position ##\vec{r} \neq \vec{0}##, because at the origin we have obviously a singularity, which is characteristic for the assumption of a "point charge" in classical field theory.
Mathematically the problem is simple because of spherical symmetry. There's no other vector in the problem than ##\vec{r}##, because no direction is in any way special except the direction of the position vector itself. Thus you can make the Ansatz
$$\vec{E} = E_r \vec{e}_r,$$
where ##\vec{e}_r=\vec{r}/r##. The "radial component" ##E_r## can only depend on ##r=|\vec{r}|##, again due to the spherical symmetry.
Now you simply use Gauss's Law in integral form
$$\int_{\partial V} \mathrm{d}^2 \vec{f} \cdot \vec{E}=Q_V/\epsilon_0.$$
It's obvious, again because of the spherical symmetry, to choose a spherical shell of radius ##r## around the origin for ##\partial V##. The surface-normal vectors are ##\vec{e}_r## and thus with our ansatz for ##\vec{E}##
$$E_r (r) 4 \ pi r^2=Q/\epsilon_0 \; \Rightarrow \; E_r(r)=\frac{Q}{4 \pi \epsilon_0 r^2}.$$
That's it! It's simply spherical symmetry and Gauss's Law!