  We analyze the near horizon conformal symmetry for black hole solutions in
gravity with a conformally coupled scalar field using the method proposed by
Majhi and Padmanabhan recently. It is shown that the entropy of the black holes
of the form $\mathrm{d}s^2 = - f(r)\mathrm{d}t^2 + \mathrm{d}r^2/f(r)+...$
agrees with Wald entropy. This result is different from previous result
obtained by M. Natsuume, T. Okamura and M. Sato using the canonical Hamiltonian
formalism, which claims a discrepancy from Wald entropy.
