“…Independently of the RTE solver, accurately accounting for the spectral behavior of the participating species entails a considerably increase on the computational time. Although Miki et al [1,2] made use of massive parallel computation of Pleiades at NASA Advanced Supercomputing facilities, solving the radiation heat transfer with the line-by-line method is prohibitive, and even accurate spectral models such as the cumulative wavenumber [16], absorption distribution function (ADF) [17,18], spectral-line moment-based [19], spectral-line-weighted-sum-of-gray gases [20][21][22][23], full-spectrum k-distribution [24,25], and variations of these last two models [26][27][28][29][30], would be excessively computer time consuming.…”