MOTIVATION
In Riemannian geometry, when one writes the metric tensor in a particular coordinate system, certain 'fake' singularities might appear that have little to do with the geometry near them.
For instance, on the sphere $S^2$, one has (with appropriate labelling)
$$ds^2 = d\phi^2 + \sin^2(\phi)d\theta^2$$
and so it looks as though the spherical metric is singular at $\phi = 0$ or $\phi = \pi/2$, but we know it is actually not. However, the only reason we know this is because we have other descriptions of this metric that are evidently not singular anywhere.
SETUP
Suppose you have a smooth manifold (let's say three-dimensional) $M$ and you are given a local description of a metric
$$ds^2 = g_{ij}dx^idx^j$$
on a coordinate patch $U \subseteq M$. If you want, you can assume this $U$ is dense in $M$, like in the sphere. Suppose that the metric looks singular near the points in $M\backslash{}U$.
Here, I mean the same type of singularity as in the sphere, that is, some crucial terms $g_{ij}$ vanish when you go away from $U$, so that the matrix $[g_{ij}]$ would have zero determinant.
Question: What are the known methods for not just detecting, but actually proving that the metric is not singular and therefore can be extended to the whole $M$?
Qiaochu's comment misses the point: Some metrics have true singularities that cannot be removed by a change of coordinates.
I don't know about general metric spaces, but in good-old 4-D space-time, a sufficient condition for a true singularity to exist at point $P$ is that the limit as one approaches the singularity of the trace of the Ricci tensor goes to infinity as one approaches $P$.
this is a fairly powerful test, but I don't remember if this is also a necessary condition; I think it is given sufficient differentiability of the metric.
It turns out that it is not sufficient (although for the Schwartzchild solution this scalar is $\frac{48G^2 M^2}{c^4r^6}$ so it does, contrary to one of the comments, tell you that the singularity at $r=0$ is true.) For metrics that are at least semi-Reimannian, the necessary and sufficient condition for non-singularity is that in the Ricci Decomposition of the curvature, all three of the following are non-singular: The scalar curvature (my original criterion); the semi-traceless part of the curvature tensor, and the fully traceless Weyl tensor. This applies in any number of dimensions above 2. I think the charged Kerr-Newman solution might pass the scalar curvature condition but fail the semi-traceless part condition at the ring of singularities.