Table 1
Detectors used to make the maps for this analysis.
Set namel | Frequency | Type | Detectors | FWHM |
[GHz] | [arcmin] | |||
|
||||
100-ds0 ......... | 100 | PSB | All 8 detectors | 9.65 |
100-ds1 ......... | 100 | PSB | 1a+1b + 4a+4b | |
100-ds2 ......... | 100 | PSB | 2a+2b + 3a+3b | |
|
||||
143-ds0 ......... | 143 | MIX | 11 detectors | 7.25 |
143-ds1 ......... | 143 | PSB | 1a+1b + 3a+3b | |
143-ds2 ......... | 143 | PSB | 2a+2b + 4a+4b | |
143-ds3 ......... | 143 | SWB | 143-5 | |
143-ds4 ......... | 143 | SWB | 143-6 | |
143-ds5 ......... | 143 | SWB | 143-7 | |
|
||||
217-ds0 ......... | 217 | MIX | 12 detectors | 4.99 |
217-ds1 ......... | 217 | PSB | 5a+5b + 7a+7b | |
217-ds2 ......... | 217 | PSB | 6a+6b + 8a+8b | |
217-ds3 ......... | 217 | SWB | 217-1 | |
217-ds4 ......... | 217 | SWB | 217-2 | |
217-ds5 ......... | 217 | SWB | 217-3 | |
217-ds6 ......... | 217 | SWB | 217-4 |
Notes. Spider web bolometers (SWB) are used individually; polarisation sensitive bolometer pairs (PSBs, denoted a and b) are used in pairs, and we consider only the maps estimated from two pairs of PSBs. The relevant effective beams, and their uncertainties, are given in Planck Collaboration VII (2014). The channel maps, or “ds0” maps, are solely used as inputs to the component separation methods, and the resulting CMB map spectra are used in Sect. 7.5 below only as a consistency check.
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