  In this paper, we study a warm intermediate inflationary model with a general
form for the dissipative coefficient $\Gamma(T,\phi)=C_\phi\,T^{m}/\phi^{m-1}$
in the context of loop quantum cosmology. We examine this model in the weak and
strong dissipative regimes. In general, we discuss in great detail the
characteristics of this model in the slow-roll approximation. Also, we assume
that the modifications to perturbation equations result exclusively from Hubble
rate. In this approach, we use recent astronomical observations from Planck and
BICEP2 experiments to restrict the parameters in our model.
