Pixel-by-pixel model for the H₂ in the transitions S(5) to S(8) toward RW Aur (emission in panels a–d) and VW Cha (emission in panels e–h), all in the MIRI-MRS field of view between band 1A to 1C. The upper rows show the resampled H₂ images (panels a-h), while the lower rows show the best model results (panels i-1 for RW Aur, and panels m-p for VW Cha). Panels (i) and (m) show the best model for H₂ S(5), panels (j) and (n) show the centroid velocity in the same line, panels (k) and (o) show the maximum likelihood slab temperature, and panels (l) and (p) show the maximum likelihood slab column density.