Fig. B.1.
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Same as Fig. 3, but for the derived dust properties (optical depth, infrared luminosity, ΣSFR, and SFE). The central ∼ 8 kpc radius is marked in the ΣSFR map and masked in the SFE map, as it is likely affected mainly by quasar heating. Some areas in the system seem to have very high SFE, with corresponding depletion times of only a few tens of Myr.
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