Table 3
APEX and IRAM 30 m CO(2-1) line fluxes and luminosities.
| GRB | Fint | S/N | Fint | log L | log L′ | log MH2,CO |
|---|---|---|---|---|---|---|
| (Jy km s−1) | (10−20 W m−2) | (L⊙) | (K km s−1 pc2) | (M⊙) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| 980425 | 5.65 ± 1.27 | 4.4 | 4.34 ± 0.98 |  |
 |
 |
| 980425_WR | 1.33 ± 1.28 | 1.0 | 1.02 ± 0.98 |  |
 |
 |
| 031203 | 7.51 ± 3.35 | 2.2 | 5.77 ± 2.58 |  |
 |
 |
| 060505 | 1.18 ± 1.64 | 0.7 | 0.91 ± 1.26 | <5.21 | <8.62 | <9.62 |
| 060814 | −0.04 ± 0.11 | −0.4 | −0.03 ± 0.09 | <6.51 | <9.92 | <10.92 |
| 080207 | 0.38 ± 0.11 | 3.5 | 0.29 ± 0.08 |  |
 |
 |
| 100316D | −0.88 ± 2.25 | −0.4 | −0.68 ± 1.73 | <4.76 | <8.16 | <9.16 |
| 111005A_CENT | 28.49 ± 2.94 | 9.7 | 21.91 ± 2.26 |  |
 |
 |
| 111005A_NW | 10.27 ± 2.13 | 4.8 | 7.90 ± 1.63 |  |
 |
 |
| 111005A_SE | 5.41 ± 1.52 | 3.5 | 4.16 ± 1.17 |  |
 |
 |
Notes. (1) GRB. (2) Integrated flux within the velocity interval shown by the dotted lines in Fig. 1. (3) Signal-to-noise ratio of the line within this velocity interval. (4) Corresponding integrated flux in W m−2. (5) Line luminosity. (6) Line luminosity in temperature units based on Eq. (3) in Solomon et al. (1997). (7) Molecular gas mass estimated assuming 
(see Sects. 2.3 and 3) and the Galactic CO-to-H2 conversion factor αCO = 5 M⊙ Kkms−1 pc2.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.