Table 2.
Complementary data used in this study and their properties.
Angular | NGC 2146 | NGC 2976 | |||
---|---|---|---|---|---|
Telescope | Wavelength | resolution | σrms | σrms | Reference |
WSRT | 21 cm | 12.5″ | 6.5 × 10−5 | 2.7 × 10−5 | Braun et al. (2007) |
WSRT | 18 cm | 10″ | 4.7 × 10−5 | 3.8 × 10−5 | Braun et al. (2007) |
Effelsberg | 6.2 cm | 144″ | 5.0 × 10−4 | 2.0 × 10−3 | Tabatabaei et al. (2017) |
Effelsberg | 2.8 cm | 69″ | – | – | Niklas et al. (1995) |
Planck | 1.38 mm | 301″ | 1.8 × 10−1 | 6.8 × 10−2 | Planck Collaboration I (2014), Clark et al. (2018) |
Herschel-SPIRE | 500 μm | 36″ | 5.3 × 10−2 | 1.4 × 10−2 | Kennicutt et al. (2011) |
Herschel-SPIRE | 350 μm | 25″ | 7.4 × 10−2 | 1.8 × 10−2 | Kennicutt et al. (2011) |
Herschel-SPIRE | 250 μm | 18″ | 1.4 × 10−1 | 7.9 × 10−2 | Kennicutt et al. (2011) |
Herschel-PACS | 160 μm | 11.4″ | 9.2 × 10−1 | 3.6 × 10−1 | Kennicutt et al. (2011) |
Herschel-PACS | 100 μm | 6.8″ | 3.7 × 100 | 9.3 × 10−1 | Kennicutt et al. (2011) |
Herschel-PACS | 70 μm | 5.6″ | 3.6 × 100 | 6.8 × 10−1 | Kennicutt et al. (2011) |
Spitzer-MIPS | 24 μm | 6″ | 5.2 × 10−3 | 8.6 × 10−4 | Engelbracht et al. (2008), Kennicutt et al. (2003) |
GALEX-FUV | 153 nm | 4.3″ | 6.3 × 10−7 | 4.2 × 10−7 | Gil de Paz et al. (2007), Clark et al. (2018) |
IRAM 30 m HERA | CO(2−1) | 13.4″ | 4.2 × 10−1 | 2.7 × 10−1 | Leroy et al. (2009) |
VLA | HI | 5″ | – | 2.7 × 100 | Walter et al. (2008) |
Notes. The first and second columns show the instrument and wavelength of each band, next to the angular resolution in the third column. The fourth column is the σrms of each band, expressed in units of Jy/beam, except for CO, which is in K km/s and for HI which is in Jy/beam m/s. The maps listed cover the whole disk of our two galaxies. Resolutions are FWHM on each map. HI data was only available for NGC 2976. The integrated flux at 2.8 cm and its corresponding uncertainty is quoted from Niklas et al. (1995) and was not measured for this work.
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