  Earlier calculations of black hole entropy in loop quantum gravity led to a
dominant term proportional to the area, but there was a correction involving
the logarithm of the area, the Chern-Simons level being assumed to be large. We
find that the calculations yield an entropy proportional to the area eigenvalue
with no such correction if the Chern-Simons level is finite, so that the area
eigenvalue can be relatively large.
