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Fig. 1.


Spectra for the eight galaxies detected in our IRAM 30 m CLoGS survey observations. For each galaxy, a pair of spectra are shown, CO(1-0) on the left panels, CO(2-1) on the right panels. The vertical axes indicate the main beam temperature Tmb in mK. The best-fitting Gaussian (or in the case of NGC 1106, two-Gaussian model) is marked where lines were detected in emission or absorption. Zero velocity corresponds to the systemic velocity of each galaxy.

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