Table 1
Summary of the observations used in this study.
| Telescope | Instrument/ | λ0/ν0 | FWHM | △ cal a |
| Filter | [′′] | [%] | ||
|
|
||||
| GALEX | FUX | 0.154 μm | 4.2 | 4.7 |
| GALEX | NUV | 0.232 μm | 5.3 | 2.8 |
| NGVS | u | 0.381 μm | 1 | 4.7 |
| NGVS | g | 0.487 μm | 1 | 4.7 |
| NGVS | i | 0.769 μm | 0.6 | 4.7 |
| NGVS | z | 0.887 μm | 1 | 9.6 |
| Spitzer | IRAC | 3.5 μm | 1.6 | 10 |
| Spitzer | IRAC | 4.5 μm | 1.7 | 10 |
| Spitzer | IRAC | 5.8 μm | 1.9 | 10 |
| Spitzer | IRAC | 8.0 μm | 2.0 | 10 |
| Spitzer | MIPS | 24 μm | 6 | 10 |
| PdBI | 12CO(1−0) | 114.8 GHz | 4.3 × 4.1 b | – |
| VLA | HI | 1.45 GHz | 14.7 × 14.3 | − |
Notes.
The calibration uncertainties are from Morrissey et al. (2007; GALEX), Raichoor et al. (2011; NGVS), Fazio et al. (2004; IRAC) and Rieke et al. (2004), Engelbracht et al. (2007), Verley et al. (2009; MIPS). We do not include calibration errors in the CO and HI data.
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.