Fig. 2
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Astronomical emission spectrum recorded by JWST and comparison with simulations of the 
dyad of 
performed using the best-fit parameters (top panel). The simulation has been performed using the same profile parameters as in Fig. 1 (T = 700 K, FWHM = 0.4 cm−1). The wavenumber residuals of the line-by-line fits are plotted in the lower panel of the figure.
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