  We extend our recent work on the quasilocal formulation of conserved charges
to a theory of gravity containing a gravitational Chern-Simons term. As an
application of our formulation, we compute the off-shell potential and
quasilocal conserved charges of some black holes in three-dimensional
topologically massive gravity. Our formulation for conserved charges reproduces
very effectively the well-known expressions on conserved charges and the
entropy expression of black holes in the topologically massive gravity.
