ex-6: rearranged the RL deconvolution description
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@ -107,14 +107,14 @@ The convolution was implemented as follow. Consider the definition of
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convolution of two functions $f(x)$ and $g(x)$:
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$$
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f*g (x) = \int \limits_{- \infty}^{+ \infty} dy f(y) g(x - y)
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f \otimes g (x) = \int \limits_{- \infty}^{+ \infty} dy f(y) g(x - y)
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$$
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Since a histogram is made of discrete values, a discrete convolution of the
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signal $s$ and the kernel $k$ must be computed. Hence, the procedure boils
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down to a dot product between $s$ and the reverse histogram of $k$ for each
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relative position of the two histograms. Namely, if $c_i$ is the $i^{\text{th}}$
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bin of the convoluted histogram:
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down to an element wise product between $s$ and the reverse histogram of $k$
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for each relative position of the two histograms. Namely, if $c_i$ is the
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$i^{\text{th}}$ bin of the convoluted histogram:
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$$
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c_i = \sum_j k_j s_{i - j}
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@ -186,7 +186,7 @@ one.
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\node [above] at (1.95,0) {$s_{i-3}$};
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\node [below] at (1.75,-1) {$k_3$};
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\end{tikzpicture}
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\caption{Dot product as a step of the convolution between the original signal
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\caption{Element wise product as a step of the convolution between the original signal
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(above) and the kernel (center). The final result is the lower
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fledging histogram.}\label{fig:dot_conv}
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}
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@ -200,7 +200,7 @@ Fast Fourier Transform. This method is based on the property of the Fourier
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transform according to which, given two functions $f(x)$ and $g(x)$:
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$$
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\hat{F}[f*g] = \hat{F}[f] \cdot \hat{F}[g]
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\hat{F}[f \otimes g] = \hat{F}[f] \cdot \hat{F}[g]
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$$
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where $\hat{F}[\quad]$ stands for the Fourier transform of its argument.
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@ -209,8 +209,8 @@ trasform of the smeared signal and the kernel, the ratio between their
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transforms and the anti-transformation of the result:
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$$
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\hat{F}[s*k] = \hat{F}[s] \cdot \hat{F}[k] \thus
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\hat{F} [s] = \frac{\hat{F}[s*k]}{\hat{F}[k]}
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\hat{F}[s \otimes k] = \hat{F}[s] \cdot \hat{F}[k] \thus
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\hat{F} [s] = \frac{\hat{F}[s \otimes k]}{\hat{F}[k]}
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$$
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Being the histogram a discrete set of data, the Discrete Fourier Transform (DFT)
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@ -302,10 +302,10 @@ the negative backwards from the end of the array (see @fig:reorder).
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}
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\end{figure}
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When $\hat{F}[s*k]$ and $\hat{F}[k]$ are computed, their normal format must be
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restored in order to use them as standard complex numbers and compute the ratio
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between them. Then, the result must return in the half-complex format for the
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inverse DFT application.
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When $\hat{F}[s \otimes k]$ and $\hat{F}[k]$ are computed, their normal format
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must be restored in order to use them as standard complex numbers and compute
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the ratio between them. Then, the result must return in the half-complex format
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for the inverse DFT application.
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GSL provides the function `gsl_fft_halfcomplex_unpack` which passes the vectors
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from half-complex format to standard complex format. The inverse procedure,
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required to compute the inverse transformation of $\hat{F}[s]$, which is not
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@ -330,42 +330,43 @@ image can be represented in terms of a transition matrix
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$P$ operating on an underlying image:
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$$
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d_i = \sum_{j} P_{i, j} u_j
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d_i = \sum_{j} u_j \, P_{i, j}
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$$
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where $u_j$ is the intensity of the underlying image at pixel $j$ and $d_i$ is
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the detected intensity at pixel $i$. In general, a matrix whose elements are
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$P_{i,j}$ describes the portion of signal from the source pixel $j$ that is
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detected in pixel $i$.
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In one dimension, the transfer function
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can be expressed in terms of the distance between the source pixel $j$ and the
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observed $i$:
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the detected intensity at pixel $i$. Hence, the matrix describes the portion of
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signal from the source pixel $j$ that is detected in pixel $i$.
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In one dimension, the transfer function can be expressed in terms of the
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distance between the source pixel $j$ and the observed $i$:
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$$
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P_{i, j} = \widetilde{P}(i-j)
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P_{i, j} = \widetilde{P}(i-j) = P_{i - j}
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$$
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In order to estimate $u_j$ given the observed $d_i$ and a known $\widetilde{P}$,
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the following iterative procedure for the estimate $\hat{u}^t_j$ of $u_j$ can
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be applied. The $t^{\text{th}}$ iteration is updated as follows:
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In order to estimate $u_j$ given {$d_i$} and $\widetilde{P}$, the following
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iterative procedure can be applied for the estimate $\hat{u}^t_j$ of $u_j$,
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where $t$ stands for the iteration number. The $t^{\text{th}}$ step is updated
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as follows:
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$$
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\hat{u}^{t+1}_j = \hat{u}^t_j \sum_i \frac{d_i}{c_i} \, P_{ij}
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\with c_i = \sum_j P_{ij} {\hat{u^t}}_j.
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\hat{u}^{t+1}_j = \hat{u}^t_j \sum_i \frac{d_i}{c_i} \, P_{i - j}
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\with c_i = \sum_j \hat{u}^t_j \, P_{i - j}
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$$
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where $c_i$ is thereby an estimation of the blurred signal obtained with the
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previous estimation of the clean signal.
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It has been shown empirically that if this iteration converges, it converges to
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the maximum likelihood solution for $u_j$.
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Writing this more generally in terms of convolution with a point spread function
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$\tilde{P}$ it becomes:
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the maximum likelihood solution for $u_j$. Writing it in terms of convolution,
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it becomes:
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$$
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\hat{u}^{t+1} = \hat {u}^{t} \cdot \left( \frac{d}{{\hat{u}^{t}} \otimes
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\widetilde{P}} \otimes \widetilde{P}^{\star} \right)
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\hat{u}^{t+1} = \hat {u}^{t} \cdot \left( \frac{d}{{\hat{u}^{t}} \otimes P}
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\otimes P^{\star} \right)
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$$
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where the division and multiplication are element wise, and
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$\widetilde{P}^{\star}$ is the flipped point spread function.
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$P^{\star}$ is the flipped point spread function.
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---
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