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Merge pull request #23 from viajani/add_starlet_l1_norm
add script starlet l1-norm
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# -*- coding: utf-8 -*- | ||
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"""STARLET L1-NORM MODULE | ||
This module contains functions for computing the starlet l1norm | ||
as defined in Eq. (1) of https://arxiv.org/pdf/2101.01542.pdf. | ||
""" | ||
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import numpy as np | ||
from astropy.stats import mad_std | ||
from lenspack.image.transforms import starlet2d | ||
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def noise_coeff(image, nscales): | ||
"""Compute the noise coefficients :math:`\sigma^{e}_{j}` | ||
to get the estimate of the noise at the scale j | ||
following Starck and Murtagh (1998). | ||
Parameters | ||
---------- | ||
image : array_like | ||
Two-dimensional input image. | ||
nscales : int | ||
Number of wavelet scales to compute. Should not exceed log2(N), where | ||
N is the smaller of the two input dimensions. | ||
Returns | ||
------- | ||
coeff_j : numpy.ndarray | ||
Values of the standard deviation of the noise at scale j | ||
""" | ||
noise_sigma = np.random.randn(image.shape[0], image.shape[0]) | ||
noise_wavelet = starlet2d(noise_sigma, nscales) | ||
coeff_j = np.array([np.std(scale) for scale in noise_wavelet]) | ||
return coeff_j | ||
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def get_l1norm_noisy(image, noise, nscales, nbins): | ||
"""Compute the starlet :math:`\ell_1`-norm of a noisy image | ||
following Eq. (1) of https://arxiv.org/abs/2101.01542. | ||
Parameters | ||
---------- | ||
image : array_like | ||
Two-dimensional input noiseless image. | ||
noise : array_like | ||
Two-dimensional input of the noise to be added to image | ||
nscales : int | ||
Number of wavelet scales to compute. Should not exceed log2(N), where | ||
N is the smaller of the two input dimensions. | ||
nbins : int | ||
Number of bins in S/N desired for the summary statistic | ||
Returns | ||
------- | ||
bins_snr, starlet_l1norm : tuple of 1D numpy arrays | ||
Bin centers in S/N and Starlet :math:`\ell_1`-norm of the noisy image | ||
""" | ||
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# add noise to noiseless image | ||
image_noisy = image + noise | ||
# perform starlet decomposition | ||
image_starlet = starlet2d(image_noisy, nscales) | ||
# estimate of the noise | ||
noise_estimate = mad_std(image_noisy) | ||
coeff_j = noise_coeff(image, nscales) | ||
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l1_coll = [] | ||
bins_coll = [] | ||
for image_j, std_co in zip(image_starlet, coeff_j): | ||
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sigma_j = std_co * noise_estimate | ||
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snr = image_j / sigma_j | ||
thresholds_snr = np.linspace(np.min(snr), np.max(snr), nbins + 1) | ||
bins_snr = 0.5 * (thresholds_snr[:-1] + thresholds_snr[1:]) | ||
digitized = np.digitize(snr, thresholds_snr) | ||
bin_l1_norm = [np.sum(np.abs(snr[digitized == i])) | ||
for i in range(1, len(thresholds_snr))] | ||
l1_coll.append(bin_l1_norm) | ||
bins_coll.append(bins_snr) | ||
return np.array(bins_coll), np.array(l1_coll) |