Table 1
List of the masks that have been used for the analyses described in this paper.
| Mask name | Sky coverage |
| [% of unmasked pixels] | |
|
|
|
| CS-SMICA891 .... | 89.0 |
| U731 ........ | 73.0 |
| CG901 ........ | 90.0 |
| CG801 ........ | 80.0 |
| CG701 ........ | 70.0 |
| CG601 ........ | 60.0 |
| CL652 ........ | 65.1 |
| CL582 ........ | 57.8 |
| CL482 ........ | 48.0 |
| CL372 ........ | 37.3 |
| CL252 ........ | 24.7 |
Notes. (1)Planck Collaboration XII (2014), (2)Planck Collaboration XV (2014). All of them have been generated at Nside = 2048, and when needed, they have been degraded to a lower resolution, as explained in the text. The CL masks have been constructed following the procedure described in Planck Collaboration XV (2014) but for different sky coverages.
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