Table 8
Masks used for the high-ℓ analysis.
| Mask | ||
| Frequency |
|
|
| [GHz] | Temperature | Polarization |
|
|
||
| 100 ............ | T66 | P70 |
| 143 ............ | T57 | P50 |
| 217 ............ | T47 | P41 |
Notes. Temperature and polarization masks used in the likelihood are identified by T and P, followed by two digits that specify the retained sky fraction (percent). As discussed in Appendix A, T masks are derived by merging apodized Galactic, CO, and extragalactic sources masks. P masks, instead, are simply given by apodized Galactic masks.
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