I often see the following:
$$\delta\left(\boldsymbol{r}-\boldsymbol{r_{0}}\right)=\frac{1}{r^{2}\sin\theta}\delta\left(r-r_{0}\right)\delta\left(\theta-\theta_{0}\right)\delta\left(\varphi-\varphi_{0}\right)\overset{?}{=}\frac{1}{2\pi r^{2}\sin\theta}\delta\left(r-r_{0}\right)\delta\left(\theta-\theta_{0}\right)$$ and I fail to see how the $1/2\pi$ factor got out of the $\varphi$ Dirac delta when we have azimuthal symmetry in a problem. How does it come about?
*Wasn't sure what to tag, but it is relevant in many areas in physics.