Planck 2015 results
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Table 10

Parameters used for astrophysical foregrounds and instrumental modelling.

Parameter Prior range Definition

.............. [0,400] Contribution of Poisson point-source power to for Planck (in μK2)
.............. [0,400] As for but at 143 GHz
.............. [0,400] As for but at 217 GHz
.............. [0,400] As for but at 143 × 217 GHz
.............. [0,200] Contribution of CIB power to at the Planck CMB frequency for 217 GHz (in μK2)
A tSZ .............. [0,10] Contribution of tSZ to at 143 GHz (in μK2)
A kSZ .............. [0,10] Contribution of kSZ to (in μK2)
ξ tSZ × CIB .............. [0,1] Correlation coefficient between the CIB and tSZ
.............. [0,50] Amplitude of Galactic dust power at = 200 at 100 GHz (in μK2)
(7 ± 2)
.............. [0,50] As for but at 143 GHz
(9 ± 2)
.............. [0,100] As for but at 143 × 217 GHz
(21 ± 8.5)
.............. [0,400] As for but at 217 GHz
(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)

.............. [0,10] Amplitude of Galactic dust power at = 500 at 100 GHz (in μK2)
(0.06 ± 0.012)
.............. [0,10] As for but at 100 × 143 GHz
(0.05 ± 0.015)
.............. [0,10] As for but at 100 × 217 GHz
(0.11 ± 0.033)
.............. [0,10] As for but at 143 GHz
(0.1 ± 0.02)
.............. [0,10] As for but at 143 × 217 GHz
(0.24 ± 0.048)
.............. [0,10] As for but at 217 GHz
(0.72 ± 0.14)

.............. [0,10] Amplitude of Galactic dust power at = 500 at 100 GHz (in μK2)
(0.14 ± 0.042)
.............. [0,10] As for but at 100 × 143 GHz
(0.12 ± 0.036)
.............. [0,10] As for but at 100 × 217 GHz
(0.3 ± 0.09)
.............. [0,10] As for but at 143 GHz
(0.24 ± 0.072)
.............. [0,10] As for but at 143 × 217 GHz
(0.6 ± 0.18)
.............. [0,10] As for but at 217 GHz
(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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