Table 7
Dust temperatures, FIR (40–120 μm) and TIR (8–1000 μm) luminosities, and dust masses derived as described in Sects. 4.1 and 4.2.
| Name | T dust | L FIR | L TIR | M dust | SFR | ||||||||||||||||||||
| K | L ⊙ | L ⊙ | 108×M⊙ | M⊙ yr-1 | |||||||||||||||||||||
|
|
|||||||||||||||||||||||||
| 005527* | 49.5 (2.2) | 1.10 (0.26)e+11 | 2.17 (0.10)e+11 | 0.23 (0.09) | 21.99 | ||||||||||||||||||||
| 015028 | 35.9 (1.0) | 2.75 (0.31)e+11 | 4.02 (0.13)e+11 | 1.10 (0.12) | 40.799 | ||||||||||||||||||||
| 021348 | 30.2 (1.0) | 3.98 (0.61)e+11 | 5.10 (0.10)e+11 | 1.45 (0.16) | 51.74 | ||||||||||||||||||||
| 080844 | 49.4 (1.9) | 3.71 (0.75)e+10 | 8.62 (0.73)e+10 | 4.03 (1.00) | 8.75 | ||||||||||||||||||||
| 082001 | 44.3 (1.0) | 8.95 (1.00)e+10 | 1.60 (0.34)e+11 | 0.21 (0.01) | 16.23 | ||||||||||||||||||||
| 092159 | 35.9 (1.2) | 3.95 (0.69)e+11 | 5.07 (0.71)e+11 | 1.80 (0.41) | 51.44 | ||||||||||||||||||||
| 093813 | 39.6 (2.8) | 3.40 (1.30)e+10 | 6.08 (0.25)e+10 | 0.14 (0.32) | 6.17 | ||||||||||||||||||||
| 143417 | 29.3 (1.0) | 7.70 (1.40)e+10 | 1.08 (0.49)e+11 | 0.79 (0.27) | 11.01 | ||||||||||||||||||||
| 210358 | 33.4 (1.0) | 2.54 (0.40)e+11 | 5.11 (0.12)e+11 | 7.2 (1.10) | 51.90 | ||||||||||||||||||||
Notes. Star-formation rates are derived from LTIR using the scaling relation given by Kennicutt & Evans (2012), divided by a factor of 1.7 to convert from the Salpeter to the Chabrier IMF that we adopt in this work.
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.