Table 2.
Results of our molecular gas observations with NOEMA.
| Galaxy | Transition | Component | Flux | Velocity | FWHM | L′line |
|---|---|---|---|---|---|---|
| (Jy km s−1) | (km s−1) | (km s−1) | (K km s−1 pc2) | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| RX 1532 | CO(3→2) | Total | 22.73 ± 0.30 | −52 ± 2 | 349 ± 6 | (1.68 ± 0.02)×1010 |
| 0 | 9.80 ± 0.09 | −78 ± 2 | 353 ± 4 | (7.26 ± 0.07)×109 | ||
| E | 3.00 ± 0.08 | −41 ± 4 | 332 ± 11 | (2.22 ± 0.06)×109 | ||
| W | 3.90 ± 0.09 | −21 ± 4 | 344 ± 10 | (2.89 ± 0.07)×109 | ||
| S | 2.20 ± 0.11 | −88 ± 8 | 311 ± 19 | (1.63 ± 0.08)×109 | ||
| MACS 1447 | CO(3→2) | Total | 4.06 ± 0.60 | −119 ± 6 | 130 ± 8 | (6.58 ± 0.72)×109 |
| 4.11 ± 0.67 | 34 ± 14 | 197 ± 29 | ||||
| 0 | 4.40 ± 0.06 | −48 ± 2 | 241 ± 3 | (3.54 ± 0.05)×109 | ||
| E | 1.85 ± 0.05 | 86 ± 3 | 257 ± 8 | (1.49 ± 0.04)×109 | ||
| W | 1.52 ± 0.04 | −127 ± 2 | 137 ± 4 | (1.22 ± 0.03)×109 | ||
| CHIPS 1911 | CO(2→1) | Total | 3.94 ± 0.40 | −181 ± 2 | 175 ± 10 | (3.46 ± 0.18)×1010 |
| 7.33 ± 0.41 | −79 ± 10 | 448 ± 14 | ||||
| 0 | 9.47 ± 0.16 | −158 ± 2 | 295 ± 7 | (2.91 ± 0.05)×1010 | ||
| N | 0.40 ± 0.04 | −38 ± 7 | 140 ± 18 | (1.23 ± 0.12)×109 | ||
Notes. Column description: (1) galaxy name; (2) molecular gas transition; (3) observed component, where “Total” stands for the total flux integrated over the full extension of the source, while 0, N, S, W, and E denote that the flux has been measured over the central, northen, southern, western, and eastern sub-regions, respectively, as illustrated in Fig. 3; (4) velocity integrated flux of the line; (5) relative velocity with respect to that corresponding to the source redshift; (6) line full width at half maximum; (7) velocity integrated line luminosity. For a given BCG and component, multiple entries for the columns (4–6) refer to Gaussian fits where two curves have been used to fit each spectrum, while one Gaussian is used instead as default.
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