  We derive a rotating counterpart of the five-dimensional electrically charged
Bardeen regular black holes spacetime by employing the Giampieri algorithm on
static one. The associated nonlinear electrodynamics source is computed in
order to justify the rotating solution. We thoroughly discuss the energy
conditions and the other properties of the rotating spacetime. The black hole
thermodynamics of the rotating spacetime is also presented. In particular, the
thermodynamic quantities such as the Hawking temperature and the heat capacity
are calculated and plotted to see the thermal behavior. The Hawking temperature
profile of the black hole implies that the regular black holes are thermally
colder than its singular counterpart. On the other hand, we find that the heat
capacity has two branches: the negative branch corresponds to the unstable
phase and the positive branch corresponds to that of the stable phase for a
suitable choice of the physical parameters characterizing the black holes.
