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.
The classification of isolated singularities can be stated through the Laurent expansion of about :
  • The singularity is removable when extends holomorphically to , equivalently when every negative-power Laurent coefficient is zero.
  • It is a pole of order when extends holomorphically to a function nonzero at . Equivalently, the Laurent series starts with a nonzero term and has no more negative power.
  • It is essential when it is neither removable nor a pole, equivalently when infinitely many negative-power coefficients are nonzero.