  The increasing interest in studying the role of holographic dark energy in
the evolution of the very early universe motivates us to study it for the
scenario of warm inflation. Due to this scenario, the holographic dark energy,
which now drives inflation, has an interaction with the radiation. The case of
interacting dark energy also has received increasing interest in studying the
late time cosmology. The Infrared cutoff is taken as the Hubble length and all
corrections are assumed to be exhibited by the parameter $c$, which appears in
the holographic dark energy. By comparing the predictions of the model with
observational data, the free constants of the model could be determined. Then,
by using these values of the constants, the energy density of inflation is
estimated. Next, we consider the validity of the fundamental assumptions of the
warm inflation, e.g. $T/H > 1$, which is necessary to be held during inflation,
for the obtained values of the constant. Gathering all outcomes, the model
could be count as a suitable candidate for warm inflation.
