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Table 3.
Percentage of diffuse background in each of the SFR tracers and atomic gas in the star-forming regions in the sample galaxies, along with the filtering scale used in Nebulosity Filter.
Galaxy | Diffuse | Filtering | |||
---|---|---|---|---|---|
background |
scale (a) | ||||
Hα | FUV | 24 μm | H I | (kpc) | |
NGC 0628 | 25 | 28 | 38 | 67 | 1.8 |
NGC 3184 | 25 | 20 | 32 | 63 | 2.7 |
NGC 3351 | 45 | 33 | 25 | 76 | 2.3 |
NGC 3521 | 22 | 45 | 17 | 80 | 1.9 |
NGC 4736 | 26 | 15 | 16 | 76 | 1.3 |
NGC 5055 | 26 | 38 | 43 | 76 | 1.9 |
NGC 5194 | 2 | 25 | 20 | 58 | 2.0 |
NGC 5457 | 5 | 14 | 23 | 37 | 2.9 |
NGC 6946 | 19 | 28 | 17 | 63 | 3.0 |
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