Image Details
Caption: Figure 10.
(a) Distribution of the velocity-integrated flux of the [Cii] line,
I
[C II], for all the galaxies in our sample. (b) Distribution of the number of detections as a function of line flux,
(computed assuming a 300 km s
−1 line width), expected in the highest frequency bands available for ALMA and PdBI/NOEMA.
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