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Table 2

Solar dipole amplitude and direction by frequency, as well as for the average (AVG) of the 100 and 143-GHz maps.

ν I857 threshold A l b
[GHz] [M Jy sr-1] [ μK] [deg] [deg]

100 ................ 2 3361.25 ± 0.06 263.937 ± 0.002 48.2647 ± 0.0008
3 3361.22 ± 0.05 263.937 ± 0.002 48.2644 ± 0.0006
4 3361.46 ± 0.04 263.942 ± 0.002 48.2634 ± 0.0006
143 ................ 2 3362.85 ± 0.04 263.913 ± 0.001 48.2629 ± 0.0004
3 3362.46 ± 0.03 263.910 ± 0.001 48.2647 ± 0.0004
4 3362.15 ± 0.02 263.914 ± 0.001 48.2664 ± 0.0003
217 ................ 2 3366.56 ± 0.06 263.852 ± 0.002 48.2645 ± 0.0008
3 3365.37 ± 0.05 263.840 ± 0.002 48.2713 ± 0.0007
4 3364.38 ± 0.04 263.846 ± 0.001 48.2765 ± 0.0006
353 ................ 2 3364.19 ± 0.26 263.385 ± 0.009 48.3191 ± 0.0035
3 3358.51 ± 0.20 263.399 ± 0.007 48.3710 ± 0.0030
4 3352.99 ± 0.18 263.452 ± 0.006 48.4207 ± 0.0028
545 ................ 2 3398.72 ± 1.99 255.890 ± 0.070 48.1571 ± 0.0281
3 3350.02 ± 1.56 255.878 ± 0.058 48.6087 ± 0.0245
4 3292.11 ± 1.38 256.181 ± 0.052 49.1146 ± 0.0232
AVG ................ 2 3362.05 ± 0.04 263.925 ± 0.001 48.2641 ± 0.0004
3 3361.84 ± 0.03 263.924 ± 0.001 48.2650 ± 0.0004
4 3361.80 ± 0.02 263.928 ± 0.001 48.2652 ± 0.0003

Notes. Here dust emission is removed using the CMB-free 857-GHz map as a template. Fits are performed using three different masks based on the I857 temperature, corresponding to 37%, 50%, and 58% of the sky. Uncertainties are purely statistical.

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