In this article, we explore the holographic Q-picture description for charged rotating black holes in five-dimensional minimal supergravity. The central charge in the Q-picture depends only on the black hole charge, therefore it can be computed from the near horizon geometry of the extremal and non-rotating counterpart. Moreover, the CFT temperatures can be identified by studying the hidden conformal symmetry, and the related gravity-CFT dictionary can be translated via thermodynamic analysis. The entropy and absorption cross section computed from both the gravity and CFT sides properly agree with each other.
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