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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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