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We study the near horizon geometry of both static and stationary extremalOliva Tempo Troncoso (OTT) black holes. For each of these cases, a set ofconsistent asymptotic conditions is introduced. The canonical generator for thestatic configuration is shown to be regular. For the rotating OTT black hole,the asymptotic symmetry is described by the time reparametrization, the chiralVirasoro and centrally extended $u(1)$ Kac-Moody algebras.

Near horizon OTT black hole asymptotic symmetries and soft hair