Wiener filter reconstruction of a Gaussian random signal.
To reproduce, run python3 demos/getting_started_1.py 0
.
Wiener filter reconstruction results for the full and partially masked data. Shown are the original signal (orange), the reconstruction (green), and one-sigma-confidence interval (gray).
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Wiener filter reconstruction of systematically and randomly masked data on a regular grid and sphere.
The same inference code is used as in ‘1D inference without masking’. Only the definitions of the signal domains and the respective masks were changed.
To reproduce, run python3 demos/getting_started_1.py 1
.
The same with a spherical domain.
To reproduce, run python3 demos/getting_started_1.py 2
.
MAP reconstruction of Poissonian random signals.
All examples use the same inference code, except for the signal domain, mask and exposure definitions.
To reproduce, run python3 demos/getting_started_2.py n
with n in (1, 2, 3).
2D regular grid domain.
Spherical domain.
Variational Bayes reconstruction of LOS data, with random and radially distributed LOS.
To reproduce, run python3 demos/getting_started_3.py n
with n in (1, 2).
The “Faraday Map” in spherical representation on a HPSpace and a GLSpace, their quadrupole projections, the uncertainty of the map, and the angular power spectrum.
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Image reconstruction of the classic “Moon Surface” image. The original image “Moon Surface” was taken from the USC-SIPI image database.
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