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Fig. 2.
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Top panels: 1.2 mm dust-continuum detections of the stacked datasets corresponding to the low-metallicity galaxies (left; 12 + log(O/H) < 8.6; three galaxies) and high-metallicity galaxies (right; 12 + log(O/H) > 8.6; seven galaxies) presented in this work. Bottom panels: CO spectral profile for the same stacked galaxies.
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