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Fig. 24
SMMJ14009+0252, a distant star-forming submm galaxy, is so heavily obscured by dust that no optical redshift could be measured. A 20 GHz scan of the 3 mm atmospheric window allowed the detection of the redshifted CO(3–2) line, confirmed by the detection of CO(5–4) in the 2 mm window. From work by Weiß et al. (2009).
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