Fig. 3
SED of SPT2132-58, including a compilation of measurements from Strandet et al. (in prep.), (filled black circles for detections, downwards triangles for 3σ upper limits) and our new ALMA Cycle 1 continuum measurement (blue filled star), and best fit by the starburst templates of the Magdis et al. (2012) model (red line). The ⟨U⟩ parameter is the mean intensity of the radiation field heating the dust compared to the solar neighbourhood.
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