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Table 3
Slope, intercept, and Pearson correlation coefficient of the correlation between dust and synchrotron polarization fraction, computed over Galactic quadrants in the Galactic plane and off the plane.
| Quadrant | | bII | < 5° | | bII | > 5° | ||||
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| Slope | Intercept | Pearson | Slope | Intercept | Pearson | |
| Q1 ........ | 0.310 | −0.551 | 0.341 | 0.280 | −0.548 | 0.288 |
| Q2 ........ | 0.355 | −0.379 | 0.470 | 0.144 | −0.687 | 0.155 |
| Q3 ........ | 0.229 | −0.646 | 0.300 | 0.101 | −0.679 | 0.091 |
| Q4 ........ | 0.135 | −0.835 | 0.170 | 0.053 | −0.818 | 0.058 |
| All ........ | 0.346 | −0.462 | 0.469 | 0.137 | −0.704 | 0.144 |
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