Pseudo Maximum Likelihood Estimation in Elliptical Theory: Effects of Misspecification
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On Multivariate Runs Tests for Randomness
On Multivariate Runs Tests for Randomness Davy Paindaveine∗ Universit´eLibre de Bruxelles, Brussels, Belgium Abstract This paper proposes several extensions of the concept of runs to the multi- variate setup, and studies the resulting tests of multivariate randomness against serial dependence. Two types of multivariate runs are defined: (i) an elliptical extension of the spherical runs proposed by Marden (1999), and (ii) an orig- inal concept of matrix-valued runs. The resulting runs tests themselves exist in various versions, one of which is a function of the number of data-based hyperplanes separating pairs of observations only. All proposed multivariate runs tests are affine-invariant and highly robust: in particular, they allow for heteroskedasticity and do not require any moment assumption. Their limit- ing distributions are derived under the null hypothesis and under sequences of local vector ARMA alternatives. Asymptotic relative efficiencies with respect to Gaussian Portmanteau tests are computed, and show that, while Marden- type runs tests suffer severe consistency problems, tests based on matrix-valued ∗Davy Paindaveine is Professor of Statistics, Universit´eLibre de Bruxelles, E.C.A.R.E.S. and D´epartement de Math´ematique, Avenue F. D. Roosevelt, 50, CP 114, B-1050 Bruxelles, Belgium, (e-mail: [email protected]). The author is also member of ECORE, the association between CORE and ECARES. This work was supported by a Mandat d’Impulsion Scientifique of the Fonds National de la Recherche Scientifique, Communaut´efran¸caise de Belgique. 1 runs perform uniformly well for moderate-to-large dimensions. A Monte-Carlo study confirms the theoretical results and investigates the robustness proper- ties of the proposed procedures. -
1 One Parameter Exponential Families
1 One parameter exponential families The world of exponential families bridges the gap between the Gaussian family and general dis- tributions. Many properties of Gaussians carry through to exponential families in a fairly precise sense. • In the Gaussian world, there exact small sample distributional results (i.e. t, F , χ2). • In the exponential family world, there are approximate distributional results (i.e. deviance tests). • In the general setting, we can only appeal to asymptotics. A one-parameter exponential family, F is a one-parameter family of distributions of the form Pη(dx) = exp (η · t(x) − Λ(η)) P0(dx) for some probability measure P0. The parameter η is called the natural or canonical parameter and the function Λ is called the cumulant generating function, and is simply the normalization needed to make dPη fη(x) = (x) = exp (η · t(x) − Λ(η)) dP0 a proper probability density. The random variable t(X) is the sufficient statistic of the exponential family. Note that P0 does not have to be a distribution on R, but these are of course the simplest examples. 1.0.1 A first example: Gaussian with linear sufficient statistic Consider the standard normal distribution Z e−z2=2 P0(A) = p dz A 2π and let t(x) = x. Then, the exponential family is eη·x−x2=2 Pη(dx) / p 2π and we see that Λ(η) = η2=2: eta= np.linspace(-2,2,101) CGF= eta**2/2. plt.plot(eta, CGF) A= plt.gca() A.set_xlabel(r'$\eta$', size=20) A.set_ylabel(r'$\Lambda(\eta)$', size=20) f= plt.gcf() 1 Thus, the exponential family in this setting is the collection F = fN(η; 1) : η 2 Rg : d 1.0.2 Normal with quadratic sufficient statistic on R d As a second example, take P0 = N(0;Id×d), i.e. -
6: the Exponential Family and Generalized Linear Models
10-708: Probabilistic Graphical Models 10-708, Spring 2014 6: The Exponential Family and Generalized Linear Models Lecturer: Eric P. Xing Scribes: Alnur Ali (lecture slides 1-23), Yipei Wang (slides 24-37) 1 The exponential family A distribution over a random variable X is in the exponential family if you can write it as P (X = x; η) = h(x) exp ηT T(x) − A(η) : Here, η is the vector of natural parameters, T is the vector of sufficient statistics, and A is the log partition function1 1.1 Examples Here are some examples of distributions that are in the exponential family. 1.1.1 Multivariate Gaussian Let X be 2 Rp. Then we have: 1 1 P (x; µ; Σ) = exp − (x − µ)T Σ−1(x − µ) (2π)p=2jΣj1=2 2 1 1 = exp − (tr xT Σ−1x + µT Σ−1µ − 2µT Σ−1x + ln jΣj) (2π)p=2 2 0 1 1 B 1 −1 T T −1 1 T −1 1 C = exp B− tr Σ xx +µ Σ x − µ Σ µ − ln jΣj)C ; (2π)p=2 @ 2 | {z } 2 2 A | {z } vec(Σ−1)T vec(xxT ) | {z } h(x) A(η) where vec(·) is the vectorization operator. 1 R T It's called this, since in order for P to normalize, we need exp(A(η)) to equal x h(x) exp(η T(x)) ) A(η) = R T ln x h(x) exp(η T(x)) , which is the log of the usual normalizer, which is the partition function. -
D. Normal Mixture Models and Elliptical Models
D. Normal Mixture Models and Elliptical Models 1. Normal Variance Mixtures 2. Normal Mean-Variance Mixtures 3. Spherical Distributions 4. Elliptical Distributions QRM 2010 74 D1. Multivariate Normal Mixture Distributions Pros of Multivariate Normal Distribution • inference is \well known" and estimation is \easy". • distribution is given by µ and Σ. • linear combinations are normal (! VaR and ES calcs easy). • conditional distributions are normal. > • For (X1;X2) ∼ N2(µ; Σ), ρ(X1;X2) = 0 () X1 and X2 are independent: QRM 2010 75 Multivariate Normal Variance Mixtures Cons of Multivariate Normal Distribution • tails are thin, meaning that extreme values are scarce in the normal model. • joint extremes in the multivariate model are also too scarce. • the distribution has a strong form of symmetry, called elliptical symmetry. How to repair the drawbacks of the multivariate normal model? QRM 2010 76 Multivariate Normal Variance Mixtures The random vector X has a (multivariate) normal variance mixture distribution if d p X = µ + WAZ; (1) where • Z ∼ Nk(0;Ik); • W ≥ 0 is a scalar random variable which is independent of Z; and • A 2 Rd×k and µ 2 Rd are a matrix and a vector of constants, respectively. > Set Σ := AA . Observe: XjW = w ∼ Nd(µ; wΣ). QRM 2010 77 Multivariate Normal Variance Mixtures Assumption: rank(A)= d ≤ k, so Σ is a positive definite matrix. If E(W ) < 1 then easy calculations give E(X) = µ and cov(X) = E(W )Σ: We call µ the location vector or mean vector and we call Σ the dispersion matrix. The correlation matrices of X and AZ are identical: corr(X) = corr(AZ): Multivariate normal variance mixtures provide the most useful examples of elliptical distributions. -
Lecture 2 — September 24 2.1 Recap 2.2 Exponential Families
STATS 300A: Theory of Statistics Fall 2015 Lecture 2 | September 24 Lecturer: Lester Mackey Scribe: Stephen Bates and Andy Tsao 2.1 Recap Last time, we set out on a quest to develop optimal inference procedures and, along the way, encountered an important pair of assertions: not all data is relevant, and irrelevant data can only increase risk and hence impair performance. This led us to introduce a notion of lossless data compression (sufficiency): T is sufficient for P with X ∼ Pθ 2 P if X j T (X) is independent of θ. How far can we take this idea? At what point does compression impair performance? These are questions of optimal data reduction. While we will develop general answers to these questions in this lecture and the next, we can often say much more in the context of specific modeling choices. With this in mind, let's consider an especially important class of models known as the exponential family models. 2.2 Exponential Families Definition 1. The model fPθ : θ 2 Ωg forms an s-dimensional exponential family if each Pθ has density of the form: s ! X p(x; θ) = exp ηi(θ)Ti(x) − B(θ) h(x) i=1 • ηi(θ) 2 R are called the natural parameters. • Ti(x) 2 R are its sufficient statistics, which follows from NFFC. • B(θ) is the log-partition function because it is the logarithm of a normalization factor: s ! ! Z X B(θ) = log exp ηi(θ)Ti(x) h(x)dµ(x) 2 R i=1 • h(x) 2 R: base measure. -
Generalized Skew-Elliptical Distributions and Their Quadratic Forms
Ann. Inst. Statist. Math. Vol. 57, No. 2, 389-401 (2005) @2005 The Institute of Statistical Mathematics GENERALIZED SKEW-ELLIPTICAL DISTRIBUTIONS AND THEIR QUADRATIC FORMS MARC G. GENTON 1 AND NICOLA M. R. LOPERFIDO2 1Department of Statistics, Texas A ~M University, College Station, TX 77843-3143, U.S.A., e-mail: genton~stat.tamu.edu 2 Instituto di scienze Econoraiche, Facoltd di Economia, Universit~ degli Studi di Urbino, Via SaJ~ 42, 61029 Urbino ( PU), Italy, e-mail: nicolaQecon.uniurb.it (Received February 10, 2003; revised March 1, 2004) Abstract. This paper introduces generalized skew-elliptical distributions (GSE), which include the multivariate skew-normal, skew-t, skew-Cauchy, and skew-elliptical distributions as special cases. GSE are weighted elliptical distributions but the dis- tribution of any even function in GSE random vectors does not depend on the weight function. In particular, this holds for quadratic forms in GSE random vectors. This property is beneficial for inference from non-random samples. We illustrate the latter point on a data set of Australian athletes. Key words and phrases: Elliptical distribution, invariance, kurtosis, selection model, skewness, weighted distribution. 1. Introduction Probability distributions that are more flexible than the normal are often needed in statistical modeling (Hill and Dixon (1982)). Skewness in datasets, for example, can be modeled through the multivariate skew-normal distribution introduced by Azzalini and Dalla Valle (1996), which appears to attain a reasonable compromise between mathe- matical tractability and shape flexibility. Its probability density function (pdf) is (1.1) 2~)p(Z; ~, ~-~) . O(ozT(z -- ~)), Z E ]~P, where Cp denotes the pdf of a p-dimensional normal distribution centered at ~ C ]~P with scale matrix ~t E ]~pxp and denotes the cumulative distribution function (cdf) of a standard normal distribution. -
Exponential Families and Theoretical Inference
EXPONENTIAL FAMILIES AND THEORETICAL INFERENCE Bent Jørgensen Rodrigo Labouriau August, 2012 ii Contents Preface vii Preface to the Portuguese edition ix 1 Exponential families 1 1.1 Definitions . 1 1.2 Analytical properties of the Laplace transform . 11 1.3 Estimation in regular exponential families . 14 1.4 Marginal and conditional distributions . 17 1.5 Parametrizations . 20 1.6 The multivariate normal distribution . 22 1.7 Asymptotic theory . 23 1.7.1 Estimation . 25 1.7.2 Hypothesis testing . 30 1.8 Problems . 36 2 Sufficiency and ancillarity 47 2.1 Sufficiency . 47 2.1.1 Three lemmas . 48 2.1.2 Definitions . 49 2.1.3 The case of equivalent measures . 50 2.1.4 The general case . 53 2.1.5 Completeness . 56 2.1.6 A result on separable σ-algebras . 59 2.1.7 Sufficiency of the likelihood function . 60 2.1.8 Sufficiency and exponential families . 62 2.2 Ancillarity . 63 2.2.1 Definitions . 63 2.2.2 Basu's Theorem . 65 2.3 First-order ancillarity . 67 2.3.1 Examples . 67 2.3.2 Main results . 69 iii iv CONTENTS 2.4 Problems . 71 3 Inferential separation 77 3.1 Introduction . 77 3.1.1 S-ancillarity . 81 3.1.2 The nonformation principle . 83 3.1.3 Discussion . 86 3.2 S-nonformation . 91 3.2.1 Definition . 91 3.2.2 S-nonformation in exponential families . 96 3.3 G-nonformation . 99 3.3.1 Transformation models . 99 3.3.2 Definition of G-nonformation . 103 3.3.3 Cox's proportional risks model . -
Elliptical Symmetry
Elliptical symmetry Abstract: This article first reviews the definition of elliptically symmetric distributions and discusses identifiability issues. It then presents results related to the corresponding characteristic functions, moments, marginal and conditional distributions, and considers the absolutely continuous case. Some well known instances of elliptical distributions are provided. Finally, inference in elliptical families is briefly discussed. Keywords: Elliptical distributions; Mahalanobis distances; Multinormal distributions; Pseudo-Gaussian tests; Robustness; Shape matrices; Scatter matrices Definition Until the 1970s, most procedures in multivariate analysis were developed under multinormality assumptions, mainly for mathematical convenience. In most applications, however, multinormality is only a poor approximation of reality. In particular, multinormal distributions do not allow for heavy tails, that are so common, e.g., in financial data. The class of elliptically symmetric distributions extends the class of multinormal distributions by allowing for both lighter-than-normal and heavier-than-normal tails, while maintaining the elliptical geometry of the underlying multinormal equidensity contours. Roughly, a random vector X with elliptical density is obtained as the linear transformation of a spherically distributed one Z| namely, a random vector with spherical equidensity contours, the distribution of which is invariant under rotations centered at the origin; such vectors always can be represented under the form Z = RU, where -
Exponential Family
School of Computer Science Probabilistic Graphical Models Learning generalized linear models and tabular CPT of fully observed BN Eric Xing Lecture 7, September 30, 2009 X1 X1 X1 X1 X2 X3 X2 X3 X2 X3 Reading: X4 X4 © Eric Xing @ CMU, 2005-2009 1 Exponential family z For a numeric random variable X T p(x |η) = h(x)exp{η T (x) − A(η)} Xn 1 N = h(x)exp{}η TT (x) Z(η) is an exponential family distribution with natural (canonical) parameter η z Function T(x) is a sufficient statistic. z Function A(η) = log Z(η) is the log normalizer. z Examples: Bernoulli, multinomial, Gaussian, Poisson, gamma,... © Eric Xing @ CMU, 2005-2009 2 1 Recall Linear Regression z Let us assume that the target variable and the inputs are related by the equation: T yi = θ xi + ε i where ε is an error term of unmodeled effects or random noise z Now assume that ε follows a Gaussian N(0,σ), then we have: 1 ⎛ (y −θ T x )2 ⎞ p(y | x ;θ) = exp⎜− i i ⎟ i i ⎜ 2 ⎟ 2πσ ⎝ 2σ ⎠ © Eric Xing @ CMU, 2005-2009 3 Recall: Logistic Regression (sigmoid classifier) z The condition distribution: a Bernoulli p(y | x) = µ(x) y (1 − µ(x))1− y where µ is a logistic function 1 µ(x) = T 1 + e−θ x z We can used the brute-force gradient method as in LR z But we can also apply generic laws by observing the p(y|x) is an exponential family function, more specifically, a generalized linear model! © Eric Xing @ CMU, 2005-2009 4 2 Example: Multivariate Gaussian Distribution z For a continuous vector random variable X∈Rk: 1 ⎧ 1 T −1 ⎫ p(x µ,Σ) = 1/2 exp⎨− (x − µ) Σ (x − µ)⎬ ()2π k /2 Σ ⎩ 2 ⎭ Moment parameter -
Tracy-Widom Limit for the Largest Eigenvalue of High-Dimensional
Tracy-Widom limit for the largest eigenvalue of high-dimensional covariance matrices in elliptical distributions Wen Jun1, Xie Jiahui1, Yu Long1 and Zhou Wang1 1Department of Statistics and Applied Probability, National University of Singapore, e-mail: *[email protected] Abstract: Let X be an M × N random matrix consisting of independent M-variate ellip- tically distributed column vectors x1,..., xN with general population covariance matrix Σ. In the literature, the quantity XX∗ is referred to as the sample covariance matrix after scaling, where X∗ is the transpose of X. In this article, we prove that the limiting behavior of the scaled largest eigenvalue of XX∗ is universal for a wide class of elliptical distribu- tions, namely, the scaled largest eigenvalue converges weakly to the same limit regardless of the distributions that x1,..., xN follow as M,N →∞ with M/N → φ0 > 0 if the weak fourth moment of the radius of x1 exists . In particular, via comparing the Green function with that of the sample covariance matrix of multivariate normally distributed data, we conclude that the limiting distribution of the scaled largest eigenvalue is the celebrated Tracy-Widom law. Keywords and phrases: Sample covariance matrices, Elliptical distributions, Edge uni- versality, Tracy-Widom distribution, Tail probability. 1. Introduction Suppose one observed independent and identically distributed (i.i.d.) data x1,..., xN with mean 0 from RM , where the positive integers N and M are the sample size and the dimension of 1 N data respectively. Define = N − x x∗, referred to as the sample covariance matrix of W i=1 i i x1,..., xN , where is the conjugate transpose of matrices throughout this article. -
Von Mises-Fisher Elliptical Distribution Shengxi Li, Student Member, IEEE, Danilo Mandic, Fellow, IEEE
1 Von Mises-Fisher Elliptical Distribution Shengxi Li, Student Member, IEEE, Danilo Mandic, Fellow, IEEE Abstract—A large class of modern probabilistic learning recent applications [13], [14], [15], this type of skewed systems assumes symmetric distributions, however, real-world elliptical distributions results in a different stochastic rep- data tend to obey skewed distributions and are thus not always resentation from the (symmetric) elliptical distribution, which adequately modelled through symmetric distributions. To ad- dress this issue, elliptical distributions are increasingly used to is prohibitive to invariance analysis, sample generation and generalise symmetric distributions, and further improvements parameter estimation. A further extension employs a stochastic to skewed elliptical distributions have recently attracted much representation of elliptical distributions by assuming some attention. However, existing approaches are either hard to inner dependency [16]. However, due to the added dependency, estimate or have complicated and abstract representations. To the relationships between parameters become unclear and this end, we propose to employ the von-Mises-Fisher (vMF) distribution to obtain an explicit and simple probability repre- sometimes interchangeable, impeding the estimation. sentation of the skewed elliptical distribution. This is shown In this paper, we start from the stochastic representation of not only to allow us to deal with non-symmetric learning elliptical distributions, and propose a novel generalisation by systems, but also to provide a physically meaningful way of employing the von Mises-Fisher (vMF) distribution to explic- generalising skewed distributions. For rigour, our extension is itly specify the direction and skewness, whilst keeping the proved to share important and desirable properties with its symmetric counterpart. -
3.4 Exponential Families
3.4 Exponential Families A family of pdfs or pmfs is called an exponential family if it can be expressed as ¡ Xk ¢ f(x|θ) = h(x)c(θ) exp wi(θ)ti(x) . (1) i=1 Here h(x) ≥ 0 and t1(x), . , tk(x) are real-valued functions of the observation x (they cannot depend on θ), and c(θ) ≥ 0 and w1(θ), . , wk(θ) are real-valued functions of the possibly vector-valued parameter θ (they cannot depend on x). Many common families introduced in the previous section are exponential families. They include the continuous families—normal, gamma, and beta, and the discrete families—binomial, Poisson, and negative binomial. Example 3.4.1 (Binomial exponential family) Let n be a positive integer and consider the binomial(n, p) family with 0 < p < 1. Then the pmf for this family, for x = 0, 1, . , n and 0 < p < 1, is µ ¶ n f(x|p) = px(1 − p)n−x x µ ¶ n ¡ p ¢ = (1 − p)n x x 1 − p µ ¶ n ¡ ¡ p ¢ ¢ = (1 − p)n exp log x . x 1 − p Define 8 >¡ ¢ < n x = 0, 1, . , n h(x) = x > :0 otherwise, p c(p) = (1 − p)n, 0 < p < 1, w (p) = log( ), 0 < p < 1, 1 1 − p and t1(x) = x. Then we have f(x|p) = h(x)c(p) exp{w1(p)t1(x)}. 1 Example 3.4.4 (Normal exponential family) Let f(x|µ, σ2) be the N(µ, σ2) family of pdfs, where θ = (µ, σ2), −∞ < µ < ∞, σ > 0.