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Table 3
Best-fit parameters of SFR vs. inclination where SFR is normalised by the MS SFR given the galaxy mass: median, 5th, and 95th percentile of the distribution.
| λ | Slope | Intercept |
|---|---|---|
| SFRUV z ~ 0 | −0.79  |
−0.20  |
| SFRMIR z ~ 0 | −0.12  |
0.05  |
| SFRFIR z ~ 0 | −0.06  |
0.67  |
| SFRradio z ~ 0 | −0.10  |
0.52  |
| SFRUV z ~ 0.7 | −0.54  |
−0.74  |
| SFRMIR z ~ 0.7 | −0.03  |
0.28  |
| SFRFIR z ~ 0.7 | −0.02  |
0.54  |
| SFRradio z ~ 0.7 | −0.17  |
0.68  |
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