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Fig. 3.
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Observables generated for the line-emission-based analysis carried out in this work. Left: Spectrum at a resolution R = 3000 in the optical 0.4 − 0.7 μm, right: Selected windows for lines in the FIR, again at R = 3000. At each of these wavelengths, we also generate images at a spatial resolution of 0.5 kpc.
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