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Table 4.

Summary of our IRAM 30 m results for the sources with secure or tentative CO detections.

Galaxy CO(J → J − 1) SCO(J → J − 1) Δv S/N FWHM zCO(J → J − 1)
(Jy km s−1) (km s−1) (109 K km s−1 pc2)
(1) (2) (3) (4) (5) (6) (7)
M0329 2→1 2.4 ± 0.7 3.3 248 ± 75 6.3 ± 1.8 0.4508 ± 0.0002
A1423 1→0 1.7 ± 0.5 3.4 886 ± 306 3.7 ± 1.1 0.2111 ± 0.0006
M1206 2→1 2.2 ± 0.7 3.1 266 ± 72 5.5 ± 1.8 0.4426 ± 0.0002
RX1532 1→0 3.0 ± 0.4 7.5 369 ± 51 20.0 ± 2.7 0.3620 ± 0.0001
RX1532 3→2 20.2 ± 1.6 12.6 390 ± 36 15.0 ± 1.2 0.3622 ± 0.0001
M2129 1→0 2.4 ± 0.7 3.4 312 ± 121 41 ± 12 0.5680 ± 0.0002
M2129 2→1 1.2 ± 0.3 4.0 98 ± 50 10.2 ± 2.6 ( † ) 0.5674 ± 0.0001

Notes. Column description: (1) BCG name; (2) CO transition; (3) integrated CO line flux; (4) signal-to-noise ratio of the CO(J → J − 1) detection; (5) full width at half maximum of the CO(J → J − 1) line; (6) CO(J → J − 1) velocity integrated luminosity; (7) redshift derived from the CO(J → J − 1) line. ( † ) The reported of M2129 is estimated from the CO(2→1) flux and has been increased by a factor of two to take into account the possibility that the fit misses a substantial part of the CO(2→1) emission.

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