  A thorough MCMC analysis of any inflationary model against the current
cosmological data is essential for assessing the validity of such a model as a
viable inflationary model. Warm Inflation, producing both thermal and quantum
fluctuations, yield a complex form of scalar power spectrum, which, in general,
cannot be directly written as a function of the comoving wavenumber $k$, an
essential step to incorporate the primordial spectra into CAMB to do an MCMC
analysis through CosmoMC/Cobaya. In this paper, we devised an efficient
generalized methodology to mould the WI power spectra as a function of $k$,
without the need of slow-roll approximation of the inflationary dynamics. The
methodology is directly applicable to any Warm Inflation model, including the
ones with complex forms of the dissipative coefficient and the inflaton
potential.
