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Fig. A.1.
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Similar to Fig. 4 but for ID2756. The 3σ upper limit at 1.3 mm is not sufficiently deep to rule out the low Tdust solution, nor to rule out the scenario without an AGN. Deeper FIR/submillimeter observations, at least similar to those for ID9094 (rms level ∼30.4 μJy beam−1 at 1.3 mm), are needed.
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