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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