Table 2
CMB solar dipole measurements for the 100 and 143 GHz channels estimated for different sky coverage levels (37, 50, and 58%) corresponding to three thresholds in 857 GHz amplitude (2, 3, and 4 MJy sr-1).
| Frequency | Threshold | d | Lon | Lat | |
| [GHz] | [ MJy sr-1] | [ μK] | [°] | [°] | |
|
|
|||||
| 100 ....................... | 2 | 3364.81 ± 0.06 | 263.921 ± 0.002 | 48.2642 ± 0.0008 | |
| 100 ....................... | 3 | 3364.76 ± 0.05 | 263.922 ± 0.002 | 48.2640 ± 0.0006 | |
| 100 ....................... | 4 | 3364.99 ± 0.04 | 263.928 ± 0.002 | 48.2631 ± 0.0006 | |
| 143 ....................... | 2 | 3364.05 ± 0.03 | 263.908 ± 0.001 | 48.2641 ± 0.0004 | |
| 143 ....................... | 3 | 3363.72 ± 0.02 | 263.903 ± 0.001 | 48.2653 ± 0.0003 | |
| 143 ....................... | 4 | 3363.39 ± 0.02 | 263.905 ± 0.001 | 48.2668 ± 0.0003 | |
Notes. Uncertainties include only statistical errors. Systematic errors are 0.8 μK for the amplitude, and (0.̊024, 0.̊0034) in Galactic (longitude, latitude).
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