  We present the computation of logarithmic corrections to near-extremal black
hole entropy from one-loop Euclidean gravity path integral around the
near-horizon geometry. We extract these corrections employing a suitably
modified heat kernel method, where the near-extremal near-horizon geometry is
treated as a perturbation around the extremal near-horizon geometry. Using this
method we compute the logarithmic corrections to non-rotating solutions in four
dimensional Einstein-Maxwell and $\mathcal{N} = 2,4,8$ supergravity theories.
We also discuss the limit that suitably recovers the extremal black hole
results.
