At the origin, the Taylor series and give
Thus has a pole of order three and a pole of order four at zero. For the third function, the Laurent series
has infinitely many nonzero negative-power terms, so zero is an essential singularity of .
To classify the point at infinity on the Riemann sphere, use the coordinate . Then
so has a simple pole at infinity.
For the other two functions, an important qualification is necessary. The poles of at nonzero integer multiples of , and those of at nonzero integer multiples of , approach infinity. Equivalently, their images in the coordinate accumulate at zero. Hence infinity is a non-isolated singularity of and . Neither function is holomorphic on any punctured neighbourhood of infinity, so the classification of isolated singularities into removable singularities, poles and essential singularities does not apply there.

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