Table 3
Velocity integrated CO(2–1) flux, luminosity, molecular gas mass, stellar mass, molecular gas-to-stellar mass ratio, and molecular gas fraction for the CARLA J1103 + 3449 cluster confirmed members.
| id | SCO Δv | LCO | Mgas | M* | Mgas∕M* | fgas |
|---|---|---|---|---|---|---|
| (Jy km s−1) | (109 Kpc2km s−1) | (1010M⊙) | (1010M⊙) | (%) | ||
| AGN/491 | <0.3 | <7 | <3 | 5 ± 2 | <0.6 | <40 |
| 490 | <0.3 | <7 | <3 | ... | ... | ... |
| 320 | < 0.4 | < 10 | < 4 | 0.7 ± 0.7 | < 6 | < 85 |
| 283 | <0.5 | <12 | <5 | ... | ... | ... |
| 279 | < 0.5 | < 12 | < 5 | ... | ... | ... |
| 199 | <0.6 | <17 | <7 | 4 ± 2 | <2 | <66 |
| 183 | <0.6 | <17 | <7 | 0.3 ± 0.3 | <23 | <96 |
Notes. The identification numbers in the column “id” are the same as in the catalog published by Noirot et al. (2018). The other columns show the velocity integrated CO(2–1) flux, luminosity, molecular gas mass, stellar mass, molecular gas-to-stellar mass ratio, and molecular gas fraction of the CARLA J1103 + 3449 spectroscopically confirmed cluster members in the cluster core. The spectroscopically confirmed members were not detected with NOEMA and we report their 3σrms upper limits.
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