Planck 2013 results
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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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