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, Sorbonne Paris Cité, 10 rue Alice Domon et Léonie Duquet, 75205 Paris Cedex, vol.13
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, Royal Observatory
, Ch. d'Écogia 16, 1290 Versoix, Switzerland 17 Institute of Space Sciences, vol.19, p.34131, 28692.
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, Spain 38 Infrared Processing and Analysis Center
, Bin the projected shear onto a grid and define? as the average shear in each pixel
, = 1 for pixels where we have information and M[i 1 , i 2 ] = 0 for pixels with no galaxies, and take a support twice larger for the shear maps and include the borders in the masked region, Set the mask M: M[i 1
, Set the maximum number of iterations to I max = 100, the maximum threshold ? max = max(| ? T P * ? |), and the minimum threshold ? min = 0
, Set i = 0, ? 0 = ? max , ? i = ? k and iterate: 8. Compute the forward transform: ? = ? T ? i
, Compute? by setting to zero the coefficients ? below the threshold ? i
, Reconstruct ? i from?: ? i = ??
Decompose ? i into its wavelet coefficients {w 1 , w 2 ,
, Reconstruct ? i by performing the backward wavelet transform from the normalised coefficients
, Perform the inverse mass relation: ? i = P? i
, Enforce the observed shear? outside the gaps: ? i = (1 ? M) ? i + M? k
, Perform the direct mass inversion: ? i = P * ? i
, Update the threshold: ? i = F(i, ? min , ? max )
, Set i = i + 1. If i < I max , return to step 8
, Set k = k + 1, ? k = ? i . If k < 3, return to step 6