Table 10
Parameters used for astrophysical foregrounds and instrumental modelling.
Parameter | Prior range | Definition |
|
||
![]() |
[0,400] | Contribution of Poisson point-source power to ![]() |
![]() |
[0,400] | As for ![]() |
![]() |
[0,400] | As for ![]() |
![]() |
[0,400] | As for ![]() |
![]() |
[0,200] | Contribution of CIB power to ![]() |
A tSZ .............. | [0,10] | Contribution of tSZ to ![]() |
A kSZ .............. | [0,10] | Contribution of kSZ to ![]() |
ξ tSZ × CIB .............. | [0,1] | Correlation coefficient between the CIB and tSZ |
![]() |
[0,50] | Amplitude of Galactic dust power at ℓ = 200 at 100 GHz (in μK2) |
(7 ± 2) | ||
![]() |
[0,50] | As for ![]() |
(9 ± 2) | ||
![]() |
[0,100] | As for ![]() |
(21 ± 8.5) | ||
![]() |
[0,400] | As for ![]() |
(80 ± 20) | ||
|
||
c 100 .............. | [0,3] | Power spectrum calibration for the 100 GHz |
(0.9990004 ± 0.001) | ||
c 217 .............. | [0,3] | Power spectrum calibration for the 217 GHz |
(0.99501 ± 0.002) | ||
y cal .............. | [0.9,1.1] | Absolute map calibration for Planck |
(1 ± 0.0025) | ||
|
||
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[0,10] | Amplitude of Galactic dust power at ℓ = 500 at 100 GHz (in μK2) |
(0.06 ± 0.012) | ||
![]() |
[0,10] | As for ![]() |
(0.05 ± 0.015) | ||
![]() |
[0,10] | As for ![]() |
(0.11 ± 0.033) | ||
![]() |
[0,10] | As for ![]() |
(0.1 ± 0.02) | ||
![]() |
[0,10] | As for ![]() |
(0.24 ± 0.048) | ||
![]() |
[0,10] | As for ![]() |
(0.72 ± 0.14) | ||
|
||
![]() |
[0,10] | Amplitude of Galactic dust power at ℓ = 500 at 100 GHz (in μK2) |
(0.14 ± 0.042) | ||
![]() |
[0,10] | As for ![]() |
(0.12 ± 0.036) | ||
![]() |
[0,10] | As for ![]() |
(0.3 ± 0.09) | ||
![]() |
[0,10] | As for ![]() |
(0.24 ± 0.072) | ||
![]() |
[0,10] | As for ![]() |
(0.6 ± 0.18) | ||
![]() |
[0,10] | As for ![]() |
(1.8 ± 0.54) |
Notes. The columns indicate the symbol for each parameter, the prior used for exploration (square brackets denote uniform priors, parentheses indicate Gaussian priors), and definitions. Beam eigenmode amplitudes require a correlation matrix to fully describe their joint prior and so do not appear in the table; they are internally marginalized over rather than explicitly sampled. This table only lists the instrumental parameters that are explored in the released version, but we do consider more parameters to assess the effects of beam uncertainties and beam leakage; see Sect. 3.4.3.
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