Table 2.
GP model: summary of the model parameters, priors, and posteriors (median with 68% intervals).
Component Covariance functiona |
Parameter | z≈8.3 | z≈9.1 | z≈10.1 | |||
---|---|---|---|---|---|---|---|
Prior | Posterior | Prior | Posterior | Prior | Posterior | ||
Sky RBF |
σ2 | − | ![]() |
− | ![]() |
− | ![]() |
l [MHz] | =80 | =80 | ![]() |
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|
Mode mixing Matérn 3/2 |
σ2 | − | ![]() |
− | ![]() |
− | ![]() |
θ [radians]b | ![]() |
![]() |
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|
δbuffer [μ s] | =0.02 | =0.02 | =0.01 | =0.01 | =0.04 | =0.04 | |
Mode mixing 2 Matérn 3/2 |
σ2 | − | − | − | − | − | ![]() |
θ [radians]b | − | − | − | − | ![]() |
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|
Excess RBF |
σ2 | − | ![]() |
− | ![]() |
− | ![]() |
l [MHz] | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
|
21 cm Learned kernelc |
σ2 | − | <0.02 | − | <0.05 | − | <0.02 |
x1 | ![]() |
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|
x2 | ![]() |
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![]() |
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|
Noise Identity |
α | ![]() |
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Notes. All variance parameters are expressed relative to the noise variance estimated from the time-differenced data. The prior ranges for the variance parameters of the different components are chosen to be very broad, having no impact on this analysis.
‘RBF’ is the radial basis function; ‘Matérn 3/2’ and ‘Matérn 5/2’ are Matérn class functions (Rasmussen & Williams 2006) with ν=3/2 and ν=5/2, respectively.
The coherence-scale of the mode mixing components is baseline dependent, as defined by the foregrounds wedge equation. The corresponding coherence-scales for each redshift bins can be seen in Figure 8.
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