Open Access
Table 2
Wavelet forward–backward splitting: pipeline round 2.
Input: Visibilities: V |
Input: Stepsize: τ (chosen artificially, such that algorithm converges) |
Input: Regularization Parameter: α |
Input: Total flux: f |
▷ Precompute needed data terms and operators |
Define a dictionary of basis functions(wavelets): Γ |
Define a forward operator: G : I ↦ FΓI (note G is linear) |
Define a data-fidelity functional: df : I ↦ Slca(V, GI) + Scph(V, ΓI) |
Precompute gradient of data-fidelity functional: df′[I] |
Define a penalty term: pen : I ↦ |support(x)| (l0-norm) |
Precompute proximal operator of penalty term: proxτ (hard thrinkage operator, Eq. (25)) |
I = initialguess |
▷ Find initial image thresholding by minimizing Eq. (26) on a predefined grid of thresholds |
Define grid of possible thresholds: ti |
for i = 1, 2, 3, … do |
Hard thresholding: ![]() |
mini = df (testi) + αpen(testi) |
Find minimum i and update initial guess ![]() |
mintot = mini |
for j = 0, 1, 2, …, J do |
for i = 1, 2, 3, … do |
Hard thresholding single scale: ![]() |
mini,j = df (testi,j) + αpen(testi,j) |
if mini,j < mintot then |
mintot = mini,j |
![]() |
▷ Start forward–backward iterations from this guess |
while stopping-rule 1 do |
while stopping-rule 2 do |
I = I - τ d f′ [I] |
I = proxτ·α(I) |
I = I·f/sum(ΓI) |
Compute Multiresolution support M = {I ≠ 0} |
Output: I is approximate minimizer to Eq. (26) |
Output: Î = ΓI is an approximation to the true sky brightness distribution |
Output: As a byproduct M is a reasonable multi-resolution support |
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