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Fig. A.2


CO(1–0) spectra of the galaxies detected with the FCRAO telescope. The spectral resolution is 13.1 or 26  km s-1, depending on the spectral shape and rms noise. The x-axis represents the recession velocity in  km s-1 and the y-axis the intensity in K in the Tmb scale. The full (red) line segment shows the line width of the CO line adopted for the determination of the velocity integrated intensity. The dashed (black) line segment is the HI line width at 20% peak level, W20. An asterisk next to the name indicates a marginal detection.

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