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Fig. 3


Distribution of the 1σ rms of ALLSMOG non-detections as a function of the targets’ stellar masses. The rms is calculated over channels of δν = 50 km s-1. The survey rms goal for non-detections is indicated for both the APEX 230 GHz (dashed line) and the IRAM 30 m 115 GHz (dot-dashed line) observations.

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