Table 2.
Derived properties of the GRG sample.
| Sr. No | Re | Re | SFR | CO(1-0) | CO(2-1) | log M(H2) | tdep | log M* |
|---|---|---|---|---|---|---|---|---|
| (arcsec) | (kpc) | (M⊙ yr−1) | (Jy km s−1) | (Jy km s−1 ) | (M⊙) | Gyr | (M⊙) | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| R1-1 | 5.4 | 7.76 | 2.95 | 14.0 | 16.3 | 10.21 | 5.49 | 11.37 |
| R1-2 | 6.1 | 4.32 | 0.19 | < 1.7 | < 2.7 | < 8.63 | < 2.24 | 10.51 |
| R1-3 | 3.6 | 5.77 | 2.45 | < 1.5 | < 7.5 | < 9.35 | < 0.91 | 10.84 |
| R2-1 | 0.96 | 1.62 | 2.07 | < 1.3 | < 2.2 | < 9.34 | < 1.05 | 10.63 |
| R2-2 | 2.2 | 3.53 | 0.91 | < 0.9 | < 1.3 | < 9.13 | < 1.48 | 10.52 |
| R2-3 | 0.78 | 0.83 | 0.09 | < 0.9 | < 1.9 | < 8.73 | < 5.96 | 11.25 |
| R2-4(2) | 15.6 | 7.78 | 0.31 | < 1.2 | < 4 | < 8.16 | < 0.47 | 11.40 |
| R2-5 | 0.7 | 1.79 | 4.64 | < 1.1 | < 1.9 | < 9.69 | < 1.06 | 11.03 |
| R2-6(1) | 0.95 | 5.63 | 170 | < 1.3 | < 2.7 | < 10.82 | < 0.39 | 11.70 |
| R2-7 | 2.4 | 5.59 | 1.44 | < 1.1 | < 1.9 | < 9.59 | < 2.70 | 11.41 |
| R2-8 | 3.3 | 8.04 | 1.48 | < 0.9 | 1.1 | 9.04 | 0.74 | 11.50 |
| R2-9(1) | 0.6 | 3.55 | 8.33 | 0.54 | < 1.1 | 10.42 | 3.15 | 10.89 |
| R1-0(1) | 0.87 | 4.37 | 48.9 | < 0.45 | < 1.6 | < 10.11 | < 0.26 | 10.87 |
| R2-0 | 5.6 | 6.70 | 0.47 | < 1.1 | < 2.7 | < 8.93 | < 1.81 | 11.46 |
Notes. Re is the half-light radius, SFR is the star formation rate, CO refers to CO flux in the respective bands, log M(H2) represents the molecular mass (log scale), tdep is the depletion time, and log M* refers to the stellar mass (log scale) of the galaxy. (1) For these sources, we observed CO(3-2) instead of CO(2-1). (2) This source was also observed by Ocaña Flaquer et al. (2010). All upper limits are computed at 3σ and assuming an FWHM = 300 km s−1.
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