Fig. 2
Rest-frame Spitzer/IRS spectra. The short-low (5.5–14 μm), short-high (10–19 μm), and long-high (19–36 μm) spectra are plotted for each galaxy. For clarity, the spectra are multiplied by the following factors 1, 2.5, 14, 100, 220, and 2000, from bottom to top. The wavelengths of the H2 rotational transitions are indicated.
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