ISBI 2013 eurobioimaging
Open Bio Image Alliance
IEEE SPS BISP TC EPFL
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Deconvolution — Making the Most of Fluorescence Microscopy

Deconvolution is one of the most common image-reconstruction tasks that arise in 3D fluorescence microscopy. The aim of this challenge is to benchmark existing deconvolution algorithms and to stimulate the community to look for novel, global and practical approaches to this problem.

The challenge will be divided into two stages: a training phase and a competition (testing) phase. It will primarily be based on realistic-looking synthetic data sets representing various sub-cellular structures. In addition it will rely on a number of common and advanced performance metrics to objectively assess the quality of the results.

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PERFORMANCE METRICS

To assess the quality of the reconstruction we provide several scripts which implement the quality metrics that will be used in the deconvolution challenge. Below we briefly describe these quality metrics and the usage of the corresponding MATLAB scripts.

Peak Signal-to-Noise Ratio (PSNR)

The PSNR is defined as $$ \textrm{PSNR}=10log_{10}(\textrm{peak}^2/\textrm{MSE}) $$ where \(\textrm{peak}\) is the peak value used in the computation and \(\textrm{MSE}\) is the mean squared error between the reconstruction and the reference image-stack. To compute it we provide the psnr.m script.

Required Input Arguments

Optional Input Arguments

Output Arguments

Normalized Mean Integrated Squared Error (NMISE)

We use a modified version of the original NMISE metric, which is better suited to the image restoration problem. It is defined as $$ \textrm{NMISE}=\frac{1}{N}\sum_{i=1}^N(x_i - f_i)^2/{f_b}_i. $$ To compute it we provide the nmisec.m script.

Required Input Arguments

Output Arguments

Structure Similarity Index (SSIM)

The structural similarity (SSIM) index is a metric for measuring the similarity between two images. A description of this metric can be found on Wikipedia. To serve the needs of the 3D reconstruction we provide the ssim3D.m script which can be applied to image volumes.

Required Input Arguments

Optional Input Arguments

Output Arguments

Total Variation Score

In this challenge we are using a quality metric based on Total Variation. The metric is defined as: $$ R=\frac{\sum_{n=1}^{N}\|(\nabla x)_n-(\nabla f)_n\|}{\sum_{n=1}^N \|(\nabla f)_n\|} $$ To compute it we provide the TVscore.m script.

Required Input Arguments

Optional Input Arguments

Output Arguments

Structure Tensor Score

This quality metric is based on the eigenvalues of the 3D Structure Tensor. It is defined as $$ R=\frac{\sum_{n=1}^{N}\mid\|(S x)_n\|_1-\|(S f)_n\|_1\mid}{\sum_{n=1}^N \|(S f)_n\|_1}, $$ where \(|(S x)_n\|_1=\sqrt{\lambda_1}+\sqrt{\lambda_2}+\sqrt{\lambda_3}\), with \(\lambda_k, k=1,2,3\) the eigevalues of the Structure Tensor at the nth voxel of the image stack. To compute it we provide the STensor_score.m script.

Required Input Arguments

Optional Input Arguments

Output Arguments

Curvature Score

This quality metric is based on the eigenvalues of the 3D Hessian operator. It is defined as $$ R=\frac{\sum_{n=1}^{N}\mid\|(H x)_n\|_F-\|(H f)_n\|_F\mid}{\sum_{n=1}^N \|(H f)_n\|_F}, $$ where \(\|(H x)_n\|_F=\sqrt{\lambda_1^2+\lambda_2^2+\lambda_3^2}\), with \(\lambda_k, k=1,2,3\) the eigevalues of the Hessian operator at the nth voxel of the image stack. To compute it we provide the Curvature_score.m script.

Required Input Arguments

Optional Input Arguments

Output Arguments

Wavelet Sparsity Index

This quality metric measures the sparsity of the input in a wavelet transform domain. To compute it we provide the wavsparseidx.m script.

Required Input Arguments

Output Arguments

Fourier Shell Correlation

The Fourier shell correlation measures the normalized cross-correlation coefficient between two image stacks over corresponding shells in the Fourier space, and is defined as $$ \mbox{FSC}\left( r \right)=\frac{\sum_{r_i\in r}\hat{f}_1(r_i)\cdot \hat{f}_2^*(r_i)}{\sqrt{\sum_{r_i\in r}{|\hat{f}_1(r_i)|}^2\cdot\sum_{r_i\in r}{|\hat{f}_2(r_i)|}^2}}, $$ where \(\hat{f}_1(r_i), \hat{f}_2(r_i)\) are the Fourier components of the two image stacks at the given spatial frequency \(r_i\). To compute it we provide the FourierShellCorrelation.m script.

Required Input Arguments

Output Arguments

Relative Energy Regain

The relative energy regain is a Fourier-based quality metric which measures the recovery of information at a range of absolute spatial frequency. For more informations about this metric we refer to the following article: Heintzmann. Estimating missing information by maximum likelihood deconvolution. Micron 38 (2007) 136-144. To compute it we provide the RelativeEnergyRegain.m script.

Required Input Arguments

Output Arguments

Important Dates

Beginning of training stage

The training stage of the 2nd edition of the challenge will begin soon. Follow this link for early registration.

July 15, 2013