Table C.1
Linear coefficients, αj, and templates used to clean individual frequency maps with SEVEM.
| Template | 44 GHz | 70 GHz | 100 GHz | 143 GHz | 217 GHz | 353 GHz |
|
|
||||||
| 30−70 | 3.65 × 10-1 | |||||
| 30−44 | 1.25 × 10-1 | − 2.35 × 10-2 | 2.14 × 10-2 | − 1.03 × 10-1 | ||
| 44−70 | 1.67 × 10-1 | 1.23 × 10-1 | 1.76 × 10-1 | |||
| 217−100 | − 0.12 × 101 | |||||
| 217−143 | 8.99 × 10-1 | |||||
| 353−143 | 4.05 × 10-3 | 9.31 × 10-3 | ||||
| 545−217 | 9.92 × 10-2 | |||||
| 545−353 | 5.21 × 10-3 | 7.52 × 10-3 | 1.84 × 10-2 | |||
| 857−545 | − 4.66 × 10-5 | − 6.67 × 10-5 | − 1.21 × 10-4 | − 5.02 × 10-4 | ||
Notes. The first column lists the templates constructed to produce clean maps. Before subtraction, the maps are smoothed to a common resolution. The (353−143) GHz template is constructed at the resolution of the 44 and 70 GHz channels, in order to clean the 44 and 70 GHz maps, respectively. For the rest of the templates, the first map used to construct the templates was filtered with the beam corresponding to the second map, and vice versa. Note that for 100, 143, and 217 GHz channels, we give the coefficients used for the largest of the two regions considered in the cleaning, which covers 97% of the sky.
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