Planck 2015 results
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Table 4

Intercalibration factors by frequency between LFI, HFI, and WMAP.

cmb Anisotropy [%]

Solar dipole [%] Commander SMICA
Frequency [ghz] (Detector) = 1 25 ≤ ≤ 100 50 ≤ ≤ 500

30 ............................................. ... –0.3a± 0.1 ...
44 ............................................ ... 0.3a± 0.1 ...
70 ............................................ 0.04a 0.0a± 0.1 0.21a± 0.06
100 ............................................ 0.03 0.09 ± 0.02 0.03 ± 0.02
143 ............................................ 0b 0; –0.1 ± 0.1 c 0b
217 ............................................ 0.20 0; 0.02 ± 0.03 c 0.28 ± 0.02
353 ............................................ 0.53 0.5 ± 0.1 0.73 ± 0.11
545 ............................................ 1.25 -1.0d 1.09 ± 1.5
WMAP 23 (K) ......................... ... 0b ...
WMAP 33 (Ka) ....................... ... 0.1 ± 0.1 ...
WMAP 41 (Q) ......................... ... 0.1 ± 0.1 ...
WMAP 61 (V) ......................... ... 0.2 ± 0.1 ...
WMAP 94 (W) ......................... –0.26 0.2 ± 0.1 0.28 ± 0.15

Notes.

(a)

LFI map rescaling factors that are incorporated in the beam transfer functions, as described in Planck Collaboration II (2016), have been applied.

(b)

Reference frequency; no intercalibration calculated.

(c)

For Commander at 143 GHz, detector set “ds1” was used as a reference (intercalibration factor = 0). The mean intercalibration factor for detectors ds2+5+6+7 was −0.1 ± 0.1. Similarly, at 217 GHz detector “1” was used as a reference (intercalibration factor = 0), and the mean intercalibration factor for detectors 2+3+4 was 0.02 ± 0.03. See table 6 in Planck Collaboration X (2016) for details.

(d)

For Commander , the effective recalibration of the 545 GHz channel measured in units of μKcmb is the product of a multiplicative calibration factor and a unit conversion correction due to revised bandpass estimation. See Sect. 5.3 in Planck Collaboration X (2016) for details.

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