  Recently it has been speculated that a set of diffeomorphisms exist which act
non-trivially on the horizon of some black holes such as Kerr and Kerr-Newman
black hole. %\cite{Haco:2018ske,Haco:2019ggi}. Using this symmetry in covariant
phase space formalism one can obtain conserved charges as surface integrals on
the horizon. Kerr-Bolt spacetime is well-known for its asymptotic topology and
has been studied widely in recent years. In this work we are going to study
Kerr-Bolt black hole and provide a holographic description of it in term of
warped conformal field theory.
