Pseudo-differential operator: Difference between revisions

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{{summarize|to|Covariance matrix#Estimation|date=February 2013}}
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In [[statistics]], sometimes the [[covariance matrix]] of a [[multivariate random variable]] is not known but has to be [[estimation theory|estimated]]. '''Estimation of covariance matrices''' then deals with the question of how to approximate the actual covariance matrix on the basis of a sample from the [[Joint probability distribution|multivariate distribution]]. Simple cases, where observations are complete, can be dealt with by using the [[sample covariance matrix]]. The sample covariance matrix (SCM) is an [[unbiased estimator|unbiased]] and [[Efficiency (statistics)|efficient estimator]] of the covariance matrix if the space of covariance matrices is viewed as an [[Differential geometry#Intrinsic versus extrinsic|extrinsic]] [[convex cone]] in '''R'''<sup>''p''&times;''p''</sup>; however, measured using the [[Symmetric space|intrinsic geometry]] of [[Positive-definite matrix|positive-definite matrices]], the SCM is a [[Biased estimator|biased]] and inefficient estimator.<ref name="Smith 2005">{{cite journal| title=Covariance, Subspace, and Intrinsic Cramér–Rao Bounds| journal=IEEE Trans. Signal Processing|date=May 2005| volume=53 |pages=1610–1630| url=http://ieeexplore.ieee.org/xpls/abs_all.jsp?arnumber=1420804&tag=1| author=Smith, Steven Thomas| issue=5| doi=10.1109/TSP.2005.845428}}</ref> In addition, if the random variable has [[normal distribution]], the sample covariance matrix has [[Wishart distribution]] and a slightly differently scaled version of it is the [[maximum likelihood estimate]]. Cases involving [[missing data]] require deeper considerations. Another issue is the [[robust statistics|robustness]] to [[outlier]]s:<ref>''Robust Estimation and Outlier Detection with Correlation Coefficients'', Susan J. Devlin, R. Gnanadesikan, J. R. Kettenring, Biometrika, Vol. 62, No. 3 (Dec., 1975), pp. 531–545</ref> "Sample covariance matrices are extremely sensitive to outliers".<ref>''Robust Statistics'', [[Peter. J. Huber]], Wiley, 1981 (republished in paperback, 2004)</ref><ref>"Modern applied statistics with S", [[William N. Venables]], [[Brian D. Ripley]], Springer, 2002, ISBN 0-387-95457-0, ISBN 978-0-387-95457-8, page 336</ref>
Statistical analyses of multivariate data often involve exploratory studies of the way in which the variables change in relation to one another and this may be followed up by explicit statistical models involving the covariance matrix of the variables. Thus the estimation of covariance matrices directly from observational data plays two roles:
:* to provide initial estimates that can be used to study the inter-relationships;
:* to provide sample estimates that can be used for model checking.
 
Estimates of covariance matrices are required at the initial stages of [[principal component analysis]] and [[factor analysis]], and are also involved in versions of [[regression analysis]] that treat the [[dependent variable]]s in a data-set, jointly with the [[independent variable]] as the outcome of a random sample.
 
==Estimation in a general context==
Given a [[Sample (statistics)|sample]] consisting of ''n'' independent observations ''x''<sub>1</sub>,..., ''x''<sub>''n''</sub> of a ''p''-dimensional [[random vector]] ''X'' &isin; '''R'''<sup>''p''&times;1</sup> (a ''p''&times;1 column-vector), an [[Bias of an estimator|unbiased]] [[estimator]] of the (''p''×''p'') [[covariance matrix]]
 
:<math>\operatorname{cov}(X) = \operatorname{E}\left[\left(X-\operatorname{E}[X])(X-\operatorname{E}[X]\right)^\mathrm{T}\right]</math>
 
is the [[Sample mean and covariance|sample covariance matrix]]
 
:<math>\mathbf{Q} = {1 \over {n-1}}\sum_{i=1}^n (x_i-\overline{x})(x_i-\overline{x})^\mathrm{T},</math>
 
where <math>\textstyle x_i</math> is the ''i''-th observation of the ''p''-dimensional random vector, and
 
:<math>\overline{x} =\left[ \begin{array} [c]{c}\bar{x}_{1}\\ \vdots\\ \bar{x}_{p}\end{array} \right]  = {1 \over {n}}\sum_{i=1}^n x_i</math>
 
is the [[Sample mean and covariance|sample mean]].
This is true regardless of the distribution of the random variable ''X'', provided of course that the theoretical means and covariances exist. The reason for the factor ''n''&nbsp;&minus;&nbsp;1 rather than ''n'' is essentially the same as the reason for the same factor appearing in unbiased estimates of [[Variance#Population_variance_and_sample_variance|sample variances]] and [[Sample mean and sample covariance|sample covariances]], which relates to the fact that the mean is not known and is replaced by the sample mean.
 
In cases where the distribution of the [[random variable]]  ''X'' is known to be within a certain family of distributions, other estimates may be derived on the basis of that assumption. A well-known instance is when the [[random variable]] ''X'' is [[multivariate normal distribution|normally distributed]]: in this case the [[maximum likelihood]] [[estimator]] of the covariance matrix is slightly different from the unbiased estimate, and is given by
 
:<math>\mathbf{Q_n} = {1 \over n}\sum_{i=1}^n (x_i-\overline{x})(x_i-\overline{x})^\mathrm{T}.</math>
 
A derivation of this result is given below. Clearly, the difference between the unbiased estimator and the maximum likelihood estimator diminishes for large ''n''.
 
In the general case, the unbiased estimate of the covariance matrix provides an acceptable estimate when the data vectors in the observed data set are all complete: that is they contain no [[missing values|missing elements]]. One approach to estimating the covariance matrix is to treat the estimation of each variance or pairwise covariance separately, and to use all the observations for which both variables have valid values. Assuming the missing data are [[missing at random]] this results in an estimate for the covariance matrix which is unbiased. However, for many applications this estimate may not be acceptable because the estimated covariance matrix is not guaranteed to be positive semi-definite. This could lead to estimated correlations having absolute values which are greater than one, and/or a non-invertible covariance matrix. 
 
When estimating the [[cross-covariance]] of a pair of signals that are [[wide-sense stationary]], missing samples do ''not'' need be random (e.g., sub-sampling by an arbitrary factor is valid).
 
==Maximum-likelihood estimation for the multivariate normal distribution==
{{main|Multivariate normal distribution}}
A random vector ''X'' &isin; '''R'''<sup>''p''</sup> (a ''p''&times;1 "column vector") has a multivariate normal distribution with a nonsingular covariance matrix Σ precisely if Σ &isin; '''R'''<sup>''p'' &times; ''p''</sup> is a [[positive-definite matrix]] and the [[probability density function]] of ''X'' is
 
:<math>f(x)=(2\pi)^{-p/2}\, \det(\Sigma)^{-1/2} \exp\left(-{1 \over 2} (x-\mu)^\mathrm{T} \Sigma^{-1} (x-\mu)\right)</math>
 
where ''μ'' ∈ '''R'''<sup>''p''&times;1</sup> is the [[expected value]] of ''X''. The [[covariance matrix]] ''Σ'' is the multidimensional analog of what in one dimension would be the [[variance]], and <math>(2\pi)^{-p/2}\det(\Sigma)^{-1/2}</math> normalizes the density <math>f(x)</math> so that it integrates to 1.
 
Suppose now that ''X''<sub>1</sub>, ..., ''X''<sub>''n''</sub> are [[statistical independence|independent]] and identically distributed samples from the distribution above.  Based on the [[observed value]]s ''x''<sub>1</sub>, ..., ''x''<sub>''n''</sub> of this [[Sample (statistics)#Mathematical description|sample]], we wish to estimate Σ.
 
===First steps===
 
The likelihood function is:
 
: <math> \mathcal{L}(\mu,\Sigma)=(2\pi)^{-np/2}\, \prod_{i=1}^n \det(\Sigma)^{-1/2} \exp\left(-{1 \over 2} (x_i-\mu)^\mathrm{T} \Sigma^{-1} (x_i-\mu)\right) </math>
 
It is fairly readily shown that the [[maximum likelihood|maximum-likelihood]] estimate of the mean vector ''μ'' is the "[[sample mean]]" vector:
 
:<math>\overline{x}=(x_1+\cdots+x_n)/n.</math>
 
See [[normal distribution#Estimation of parameters|the section on estimation in the article on the normal distribution]] for details; the process here is similar.
 
Since the estimate <math>\bar{x}</math> does not depend on Σ, we can just substitute it for ''μ'' in the [[likelihood function]], getting
 
: <math>\mathcal{L}(\overline{x},\Sigma) \propto \det(\Sigma)^{-n/2} \exp\left(-{1 \over 2} \sum_{i=1}^n (x_i-\overline{x})^\mathrm{T} \Sigma^{-1} (x_i-\overline{x})\right),</math>
 
and then seek the value of &Sigma; that maximizes the likelihood of the data (in practice it is easier to work with log&nbsp;<math>\mathcal{L}</math>).
 
===The trace of a 1 &times; 1 matrix===
 
Now we come to the first surprising step: regard the [[scalar (mathematics)|scalar]] <math>(x_i-\overline{x})^\mathrm{T} \Sigma^{-1} (x_i-\overline{x})</math> as the [[trace (matrix)|trace]] of a 1&times;1 matrix.
 
This makes it possible to use the identity tr(''AB'') = tr(''BA'') whenever ''A'' and ''B'' are matrices so shaped that both products exist.
We get
 
:<math>
\mathcal{L}(\overline{x},\Sigma)\propto \det(\Sigma)^{-n/2} \exp\left(-{1 \over 2} \sum_{i=1}^n \operatorname{tr}((x_i-\overline{x})^\mathrm{T} \Sigma^{-1} (x_i-\overline{x})) \right)</math>
 
:<math>=\det(\Sigma)^{-n/2} \exp\left(-{1 \over 2} \sum_{i=1}^n \operatorname{tr}((x_i-\overline{x}) (x_i-\overline{x})^\mathrm{T} \Sigma^{-1}) \right)</math>
 
(so now we are taking the trace of a ''p''&times;''p'' matrix)
 
:<math>=\det(\Sigma)^{-n/2} \exp\left(-{1 \over 2} \operatorname{tr} \left( \sum_{i=1}^n (x_i-\overline{x}) (x_i-\overline{x})^\mathrm{T} \Sigma^{-1} \right) \right)</math>
 
:<math>=\det(\Sigma)^{-n/2} \exp\left(-{1 \over 2} \operatorname{tr} \left( S \Sigma^{-1} \right) \right)</math>
 
where
 
:<math>S=\sum_{i=1}^n (x_i-\overline{x}) (x_i-\overline{x})^\mathrm{T} \in \mathbf{R}^{p\times p}.</math>
<math>S</math> is sometimes called the [[scatter matrix]], and is positive definite if there exists a subset of the data consisting of <math>p</math> linearly independent observations (which we will assume).
 
===Using the spectral theorem===
 
It follows from the [[spectral theorem]] of [[linear algebra]] that a positive-definite symmetric matrix ''S'' has a unique positive-definite symmetric square root ''S''<sup>1/2</sup>.  We can again use the [[trace (matrix)|"cyclic property"]] of the trace to write
 
:<math>\det(\Sigma)^{-n/2} \exp\left(-{1 \over 2} \operatorname{tr} \left( S^{1/2} \Sigma^{-1} S^{1/2} \right) \right).</math>
 
Let ''B'' = ''S''<sup>1/2</sup> ''Σ''<sup> &minus;1</sup> ''S''<sup>1/2</sup>.  Then the expression above becomes
 
:<math>\det(S)^{-n/2} \det(B)^{n/2} \exp\left(-{1 \over 2} \operatorname{tr} (B) \right).</math>
 
The positive-definite matrix ''B'' can be diagonalized, and then the problem of finding the value of ''B'' that maximizes
 
:<math>\det(B)^{n/2} \exp\left(-{1 \over 2} \operatorname{tr} (B) \right)</math>
 
Since the trace of a square matrix equals the sum of eigen-values ([[Trace_(matrix)#Eigenvalue_relationships|"trace and eigenvalues"]]), the equation reduces to the problem of finding the eigen values λ<sub>1</sub>, ..., λ<sub>''p''</sub> that maximize
 
:<math>\lambda_i^{n/2} \exp(-\lambda_i/2).</math>
 
This is just a calculus problem and we get λ<sub>''i''</sub> = ''n'' for all ''i.'' Thus, assume ''Q'' is the matrix of eigen vectors, then
 
:<math>B = Q (n I_p) Q^{-1} = n I_p </math>
 
i.e., ''n'' times the ''p''&times;''p'' identity matrix.
 
===Concluding steps===
 
Finally we get
 
:<math>\Sigma=S^{1/2} B^{-1} S^{1/2}=S^{1/2}((1/n)I_p)S^{1/2}=S/n,\,</math>
 
i.e., the ''p''&times;''p'' "sample covariance matrix"
 
:<math>{S \over n} = {1 \over n}\sum_{i=1}^n (X_i-\overline{X})(X_i-\overline{X})^\mathrm{T}</math>
 
is the maximum-likelihood estimator of the "population covariance matrix" ''&Sigma;''.  At this point we are using a capital ''X'' rather than a lower-case ''x'' because we are thinking of it "as an estimator rather than as an estimate", i.e., as something random whose probability distribution we could profit by knowing.  The random matrix ''S'' can be shown to have a [[Wishart distribution]] with ''n'' &minus; 1 degrees of freedom.<ref>
[[Kanti Mardia|K.V. Mardia]], [[John Kent (statistician)|J.T. Kent]], and [[John Bibby (mathematician)|J.M. Bibby]] (1979) ''[[Multivariate Analysis]]'', [[Academic Press]].
</ref> That is:
 
:<math>\sum_{i=1}^n (X_i-\overline{X})(X_i-\overline{X})^\mathrm{T} \sim W_p(\Sigma,n-1).</math>
 
===Alternative derivation===
 
An alternative derivation of the maximum likelihood estimator can be performed via [[matrix calculus]] formulae (see also [[Determinant#Derivative|differential of a determinant]] and [[Invertible matrix#Derivative of the matrix inverse|differential of the inverse matrix]]). It also verifies the aforementioned fact about the maximum likelihood estimate of the mean. Re-write the likelihood in the log form using the trace trick:
 
:<math>\ln \mathcal{L}(\mu,\Sigma) = \operatorname{const} -{n \over 2} \ln \det(\Sigma) -{1 \over 2} \operatorname{tr}  \left[ \Sigma^{-1} \sum_{i=1}^n (x_i-\mu) (x_i-\mu)^\mathrm{T} \right]. </math>
 
The differential of this log-likelihood is
 
:<math>d \ln \mathcal{L}(\mu,\Sigma) = -{n \over 2} \operatorname{tr} \left[ \Sigma^{-1} \left\{ d \Sigma \right\} \right]</math>
:<math> -{1 \over 2} \operatorname{tr} \left[ - \Sigma^{-1} \{ d \Sigma \} \Sigma^{-1} \sum_{i=1}^n (x_i-\mu)(x_i-\mu)^\mathrm{T} - 2 \Sigma^{-1} \sum_{i=1}^n (x_i - \mu) \{ d \mu \}^\mathrm{T} \right]. </math>
 
It naturally breaks down into the part related to the estimation of the mean, and to the part related to the estimation of the variance. The [[first order condition]] for maximum, <math>d \ln \mathcal{L}(\mu,\Sigma)=0</math>, is satisfied when the terms multiplying <math>d \mu</math> and <math>d \Sigma</math> are identically zero. Assuming (the maximum likelihood estimate of) <math>\Sigma</math> is non-singular, the first order condition for the estimate of the mean vector is
 
:<math> \sum_{i=1}^n (x_i - \mu) = 0,</math>
 
which leads to the maximum likelihood estimator
 
:<math>\widehat \mu = \bar X = {1 \over n} \sum_{i=1}^n X_i.</math>
 
This lets us simplify <math>\sum_{i=1}^n (x_i-\mu)(x_i-\mu)^\mathrm{T} = \sum_{i=1}^n (x_i-\bar x)(x_i-\bar x)^\mathrm{T} = S</math> as defined above. Then the terms involving <math>d \Sigma</math> in <math>d \ln L</math> can be combined as
 
:<math> -{1 \over 2} \operatorname{tr} \left( \Sigma^{-1} \left\{ d \Sigma \right\} \left[ nI_p - \Sigma^{-1} S \right] \right). </math>
 
The first order condition <math>d \ln \mathcal{L}(\mu,\Sigma)=0</math> will hold when the term in the square bracket is (matrix-valued) zero. Pre-multiplying the latter by <math>\Sigma</math> and dividing by <math>n</math> gives
 
:<math>\widehat \Sigma = {1 \over n} S,</math>
 
which of course coincides with the canonical derivation given earlier.
 
Dwyer <ref name="Thomas 2007">{{cite journal| title=Some applications of matrix derivatives in multivariate analysis| journal=Journal of the American Statistical Association|date=June 1967| volume=62 |pages=607–625| doi=10.2307/2283988| author=Dwyer, Paul S.| issue=318| publisher=Journal of the American Statistical Association, Vol. 62, No. 318| jstor=2283988}}</ref> points out that decomposition into two terms such as appears above is "unnecessary" and derives the estimator in two lines of working. Note that it may be not trivial to show that such derived estimator is the unique global maximizer for likelihood function.
<!--
==Maximum likelihood estimation: general case==
{{main|Maximum likelihood}}
The first-order conditions for a MLE of parameter ''&theta;'' are that the first derivative of the log-likelihood function should be null at ''&theta;''<sub>MLE</sub>. Intuitively, the second derivative of the log-likelihood function indicates its curvature : the higher it is, the better identified ''&theta;''<sub>MLE</sub> since the likelihood function will be inverse-V-shaped around ''&theta;''<sub>MLE</sub>.
Formally, it can be proved that
 
:<math>\sqrt{T}(\theta_\text{MLE}-\theta) \rightarrow \mathcal{N}(0,\Omega) \, </math>
 
where <math>\Omega</math> can be estimated by
 
:<math>\left(-\frac{1}{T}\sum_{t=1}^\mathrm{T} \frac{\partial^2 \ell_t}{\partial \theta \, \partial \theta '} (\theta_\text{MLE})\right)^{-1}.</math> -->
 
==Intrinsic covariance matrix estimation==
 
===Intrinsic expectation===
 
Given a [[Sample (statistics)|sample]] of ''n'' independent observations ''x''<sub>1</sub>,..., ''x''<sub>''n''</sub> of a ''p''-dimensional zero-mean Gaussian random variable ''X'' with covariance '''R''', the [[maximum likelihood]] [[estimator]] of '''R''' is given by
 
:<math>\hat{\mathbf{R}} = {1 \over n}\sum_{i=1}^n x_ix_i^\mathrm{T}.</math>
 
The parameter '''R''' belongs to the set of [[Positive-definite matrix|positive-definite matrices]], which is a [[Riemannian manifold]], not a [[vector space]], hence the usual vector-space notions of [[Expected value|expectation]], i.e. "E['''R'''^]", and [[estimator bias]] must be generalized to manifolds to make sense of the problem of covariance matrix estimation. This can be done by defining the expectation of an manifold-valued estimator '''R'''^ with respect to the manifold-valued point '''R''' as
 
:<math>\mathrm{E}_{\mathbf{R}}[\hat{\mathbf{R}}]\ \stackrel{\mathrm{def}}{=}\ \exp_{\mathbf{R}}\mathrm{E}\left[\exp_{\mathbf{R}}^{-1}\hat{\mathbf{R}}\right]</math>
 
where
 
:<math>\exp_{\mathbf{R}}(\hat{\mathbf{R}}) =\mathbf{R}^{\frac{1}{2}}\exp\left(\mathbf{R}^{-\frac{1}{2}}\hat{\mathbf{R}}\mathbf{R}^{-\frac{1}{2}}\right)\mathbf{R}^{\frac{1}{2}}</math>
:<math>\exp_{\mathbf{R}}^{-1}(\hat{\mathbf{R}}) =\mathbf{R}^{\frac{1}{2}}\left(\log\mathbf{R}^{-\frac{1}{2}}\hat{\mathbf{R}}\mathbf{R}^{-\frac{1}{2}}\right)\mathbf{R}^{\frac{1}{2}}</math>
 
are the [[exponential map]] and inverse exponential map, respectively, "exp" and "log" denote the ordinary [[matrix exponential]] and [[matrix logarithm]], and E[·] is the ordinary expectation operator defined on a vector space, in this case the [[tangent space]] of the manifold.<ref name="Smith 2005"/>
 
===Bias of the sample covariance matrix===
 
The [[intrinsic bias]] [[vector field]] of the SCM estimator '''R'''^ is defined to be
 
:<math>\mathbf{B}(\hat{\mathbf{R}}) =\exp_{\mathbf{R}}^{-1}\mathrm{E}_{\mathbf{R}}\left[\hat{\mathbf{R}}\right] =\mathrm{E}\left[\exp_{\mathbf{R}}^{-1}\hat{\mathbf{R}}\right]</math>
 
The intrinsic estimator bias is then given by <math>\exp_{\mathbf{R}}\mathbf{B}(\hat{\mathbf{R}})</math>.
 
For [[Complex number|complex]] Gaussian random variables, this bias vector field can be shown<ref name="Smith 2005"/> to equal
 
:<math>\mathbf{B}(\hat{\mathbf{R}}) =-\beta(p,n)\mathbf{R}</math>
 
where
 
:<math>\beta(p,n) =\frac{1}{p}\left(p\log n + p -\psi(n-p+1) +(n-p+1)\psi(n-p+2)  +\psi(n+1) -(n+1)\psi(n+2)\right)</math>
 
and ψ(·) is the [[digamma function]]. The intrinsic bias of the sample covariance matrix equals
 
:<math>\exp_{\mathbf{R}}\mathbf{B}(\hat{\mathbf{R}}) =e^{-\beta(p,n)}\mathbf{R}</math>
 
and the SCM is asymptotically unbiased as ''n'' → ∞.
 
Similarly, the intrinsic [[Efficiency (statistics)|inefficiency]] of the sample covariance matrix depends upon the [[Riemannian curvature]] of the space of positive-define matrices.
 
==Shrinkage estimation==
 
If the sample size ''n'' is small and the number of considered variables ''p'' is large, the above empirical estimators of covariance and correlation are very unstable.  Specifically, it is possible to furnish estimators that improve considerably upon the maximum likelihood estimate in terms of mean squared error.  Moreover, for ''n''&nbsp;<&nbsp;''p'', the empirical estimate of the covariance matrix becomes [[singular matrix|singular]], i.e. it cannot be inverted to compute the [[precision matrix]].
 
As an alternative, many methods have been suggested to improve the estimation of the covariance matrix.  All of these approaches rely on the concept of shrinkage.  This is implicit in [[Bayesian method]]s and in penalized [[maximum likelihood]] methods and explicit in the [[James–Stein estimator|Stein-type shrinkage approach]].
 
A simple version of a shrinkage estimator of the covariance matrix is constructed as  follows. One considers a [[convex combination]] of the empirical estimator (<math>A</math>) with some suitable chosen target (<math>B</math>), e.g., the diagonal matrix.  Subsequently, the mixing parameter (<math>\delta</math>) is selected  to maximize the expected accuracy of the shrunken estimator. This can be done by [[cross-validation (statistics)|cross-validation]], or by using an analytic estimate of the shrinkage intensity. The resulting regularized estimator (<math>\delta A + (1 - \delta) B</math>) can be shown to outperform the maximum likelihood estimator for small samples.  For large samples, the shrinkage intensity will reduce to zero, hence in this case the shrinkage estimator will be identical to the empirical estimator.  Apart from increased efficiency the shrinkage estimate has the additional advantage that it is always positive definite and well conditioned.
 
A review on this topic is given, e.g., in Schäfer and Strimmer 2005.<ref>
J. Schäfer and K. Strimmer (2005) ''[http://www.bepress.com/sagmb/vol4/iss1/art32 A Shrinkage Approach to Large-Scale Covariance Matrix Estimation and Implications for Functional Genomics]'', Statistical Applications in Genetics and Molecular Biology: Vol. 4: No. 1, Article 32.</ref> A covariance shrinkage estimator is implemented in the [[R programming language|R]] package [http://cran.r-project.org/web/packages/corpcor/index.html "corpcor"] and the [http://scikit-learn.org/stable/modules/covariance.html scikit-learn] library for the [[Python programming language|Python (programming language)]].
 
==See also==
*[[Propagation of uncertainty]]
*[[Sample mean and sample covariance]]
 
==References==
<references/>
{{statistics|correlation|state=expanded}}
 
{{DEFAULTSORT:Estimation Of Covariance Matrices}}
[[Category:Estimation for specific parameters]]
[[Category:Statistical deviation and dispersion]]

Latest revision as of 07:58, 25 November 2014

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