Fig. 3.
CO(1→0) and CO(3→2) baseline-subtracted spectra of the RX1532 BCG, obtained with the IRAM 30 m. In both panels, the solid line shows the Gaussian best fit. In both panels the flux (y-axis) is plotted against the relative velocity with respect to the BCG redshift, as in Table 1 (bottom x-axis) and the observer frame frequency (top x-axis).
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