Fig. A.1
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Example of a MRS background spectrum observed at Galactic coordinates l, b = 12.881°, 0.518° (Program ID: 01290, Observation ID: 078). Top panel: Observed specific intensity as a function of wavelength, after stitching the channel-specific spectra. Bottom panels: Continuum-subtracted intensity in zoomed-in windows centered on each H2 rotational line. Detected lines are highlighted in red.
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