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Table 4
Projection coefficients used by the two likelihood methods described in Sect. 6, as well as SMICA, for removal of dust and synchrotron emission using the 353- and 30-GHz maps, respectively.
| Dust | Synchrotron | |||||||||||||
|
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| Frequency | Lollipop | SimBaL | SMICA | mean | error | Lollipop | SimBaL | SMICA | mean | error | ||||
| [GHz] | ||||||||||||||
|
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| 70 ........... | 0.0084 | 0.0060 | 0.0095 | 0.0080 | 16.7% | 0.0679 | 0.0520 | 0.0621 | 0.0621 | 16% | ||||
| 100 ......... | 0.0183 | 0.0193 | 0.0183 | 0.0186 | 4.4% | 0.0390 | 0.0200 | 0.0210 | 0.0267 | 20% | ||||
| 143 ......... | 0.0399 | 0.0427 | 0.0399 | 0.0408 | 2.3% | 0.0199 | 0.0076 | 0.0080 | 0.0118 | 45% | ||||
Notes. In all these cases, fsky = 0.5.
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