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Fig. 3.

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CO SLEDs of the ULIRGs classified as having lower excitation (left panel) and higher excitation (right panel) gas, following the classification criteria described in Sect. 3.2. Each source is shown in a different color, according to the legend reported on the top of each panel. The average CO SLED of each group of galaxies is also computed and plotted using black square symbols connected by a black solid line.

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