  This paper deals with a spatially homogeneous and totally anisotropic Bianchi
type-V cosmological model within the framework of self interacting Brans Dicke
theory of gravity in the background of anisotropic dark energy (DE) with
variable equation of state (EoS) parameter and constant deceleration parameter.
Constant deceleration parameter leads to two models of universe, i.e. power law
model and exponential model. EoS parameter {\omega} and its existing range for
the models is in good agreement with the most recent observational data. We
notice that {\omega} given by (37) i.e {\omega}(t) = log(k1t) is more suitable
in explaining the evolution of the universe. The physical behaviors of the
solutions have also been discussed using some physical quantities. Finally, we
observe that despite having several prominent features, both of the DE models
discussed fail in details.
