Abstract

Marginal probability density and cumulative distribution functions are presented for multidimensional variables defined by nonsingular affine transformations of vectors of independent two-piece normal variables, the most important subclass of Ferreira and Steel's general multivariate skewed distributions. The marginal functions are obtained by first expressing the joint density as a mixture of Arellano-Valle and Azzalini's unified skew-normal densities and then using the property of closure under marginalization of the latter class.

1. Introduction

In the literature on probability distributions, there are several approaches for extending the multivariate normal distribution with the introduction of some sort of skewness. Arellano-Valle et al. [1] provide a unified view of this literature. The largest group of contributions was initiated by Azzalini and Dalla Valle [2] and Azzalini and Capitanio [3] and generalizes the univariate skew-normal (SN) distribution studied by Azzalini [4, 5]. These “multivariate skew-normal distributions” are generated from a normal distribution either by conditioning on a truncated variable or by a convolution mechanism.

An alternative approach was proposed by Ferreira and Steel [68] and is based on nonsingular affine transformations of random vectors with independent components, each having a skewed distribution with probability density function (pdf) constructed from a symmetric distribution using the inverse scaling factor method introduced by Fernández and Steel [9]. (Arellano-Valle et al. [10] consider a general class of asymmetric univariate distributions that includes the distributions generated according to the procedure proposed by Fernández and Steel [9] as a special case.) If the univariate symmetric distribution is the standard normal, then the corresponding univariate skewed distribution becomes (with a different parameterization) the two-piece normal (tpn) analyzed by John [11] (see also Johnson et al. [12]). To overcome an issue of overparameterization, Ferreira and Steel [7, 8] pay particular attention to the subclass associated with transformation matrices that can be factorized as the product of an orthogonal matrix and a diagonal positive definite matrix. Villani and Larsson [13] studied this subclass when the basic univariate skewed distribution is the tpn and named these distributions “multivariate split normal.”

Under the acronym SUN (standing for “unified skew-normal”), Arellano-Valle and Azzalini [14] suggested a formulation for the first approach that encompasses the most relevant coexisting variants of multivariate skew-normal distributions. Like the multivariate normal and SN distributions, the class of SUN distributions is closed under affine transformations, marginalization, and conditioning to given values of some components. Besides these important properties, the SUN class is also closed under sums of independent components. However, one limitation of the SUN distributions is that the vector of location parameters does not have a direct interpretation as the mean or the mode of the distribution, which are rather complicated functions of all the parameters. Even in the simplest case of the basic SN, both the mean and the mode (for which there is no closed expression) depend on the parameters regulating dispersion and skewness.

Ferreira and Steel’s independent components approach to the construction of multivariate skewed normal distributions (henceforth FS-SN) provides an alternative to the SUN class in applications for which it is important to have some location measure that does not depend on the dispersion and skewness parameters. Indeed, the FS-SN distributions have the convenient feature that the mode is part of the distribution parameters and therefore is invariant to dispersion and skewness. In addition, the FS-SN distributions are closed under nonsingular affine transformations. However, unlike the SUN class, the FS-SN distributions are not closed under marginalization (neither under conditioning) and, to my knowledge, general closed expressions of their marginal pdf and cumulative distribution function (cdf) are not available in the literature.

This paper aims at filling the gap and proposing expressions for the marginal density and cumulative distribution functions of an FS-SN distribution. Obviously, the expressions will also apply to the subclass of multivariate split normal distributions studied by Villani and Larsson [13]. The technique used to derive the marginal distributions is simple and consists of expressing the joint FS-SN distribution as a finite mixture of singular SUN distributions and then making use of their property of closure under marginalization.

An area of application of the results presented in this paper is macroeconomic density forecasting. Many institutions that publish macroeconomic forecasts complement their point forecasts with information on the dispersion and skewness of the probability distributions of the forecasting errors. Fan charts are one of the most popular tools to convey the predictive densities, and they gained prominence through their use in inflation reports released by many central banks, with the Bank of England and the Sveriges Riksbank (the Swedish central bank) featuring as pioneers in this respect [15, 16] (see also Wallis [17, 18] and Tay and Wallis [19]). The characterization of the forecast densities is complicated by the fact that typically institutional forecasts are not based on a single model but stem from different competing models combined with judgements by experts (the latter regarding, in particular, the skewness, i.e., the balance of upward and downward risks to the forecasts). Most of the procedures used to generate the fan charts take the point baseline forecasts as given and assume that the sources of uncertainty and asymmetry have univariate tpn distributions. These sources of forecasting error are then aggregated according to a linear mapping, envisaged as an approximation around the baseline to the underlying unknown data generating process. In the absence of closed expressions for the exact distribution of a linear combination of tpn variables, some aggregation procedures resort to informal approximations based on the first moments, while other procedures are based on numerical simulation. Examples of the first approach are Blix and Sellin [16, 20, 21] and Elekdag and Kannan [22], while Pinheiro and Esteves [23] opted to simulate the distribution. The results presented in Section 3 allow to overcome this aggregation difficulty.

2. The SUN and the FS-SN Distributions

If the M-dimensional random vector 𝐘𝑆𝑈𝑁𝑀,𝑁(𝝃,𝜸,𝝎,Ω), then its pdf and cdf are, respectively, for any point 𝐲𝑅𝑀𝑔𝐘𝐲𝝃,𝜸,𝝎,𝛀=𝜑𝑀𝚽(𝐲𝝃𝛀)𝑁𝜸+𝚫𝛀𝟏𝝎𝟏(𝐲𝝃)𝚪𝚫𝛀𝟏𝚫𝚽𝑁(𝜸𝚪),(2.1)𝐺𝐘𝐲𝝃,𝜸,𝝎,𝛀=𝚽𝑁+𝑀𝜸𝝎1(𝐲𝝃)𝛀𝚽𝑁(𝜸𝚪),(2.2) where 𝜑𝑀(𝐲𝝃Ω) and Φ𝑀(𝐲𝝃Ω) denote, respectively, the pdf and the cdf at point 𝐲 of a normal distribution 𝑁𝑀(𝝃,Ω), 𝝃(𝑀×1) and 𝜸(𝑁×1) are vectors of parameters, Ω(𝑀×𝑀) is a positive definite covariance matrix, 𝝎(𝑀×𝑀) is the diagonal matrix formed by the standard deviations of Ω, Ω(𝑀×𝑀) is the correlation matrix associated with Ω (hence Ω=𝝎Ω𝝎), 𝝎=𝝎𝜾𝑁 with 𝜾𝑁=[11](𝑁×1), Γ(𝑁×𝑁) is a positive definite correlation matrix, and Δ(𝑀×𝑁) is such that𝛀=𝚪𝚫𝚫𝛀((𝑁+𝑀)×(𝑁+𝑀))(2.3) is also a (semi-definite positive) correlation matrix. (Arellano-Valle and Azzalini [14, Appendix C] consider three cases of singular SUN distributions: (i) Ω singular; (ii) Γ singular; (iii) Ω singular with nonsingular Ω and Γ. For our purposes, only the latter case is relevant.) The SUN distribution collapses to the multivariate normal when Δ=𝟎, Δ being the matrix of parameters that regulate skewness. It collapses to the basic multivariate SN distribution suggested by Azzalini and Dalla Valle [2] when 𝑁=1 and 𝜸=𝟎 (implying that Γ=1).

Now let the scalar random variable 𝑈𝑛 be tpn distributed with zero mode. Its pdf may be parameterized as follows:𝑓𝑈𝑛𝑢𝑛𝜔𝑛,𝜃𝑛=2𝜔𝑛1𝜃𝑛+𝜃𝑛11𝜙𝜔𝑛1𝜃𝑛𝑢𝑛𝑢𝑛,02𝜔𝑛1𝜃𝑛+𝜃𝑛11𝜙𝜔𝑛1𝜃𝑛1𝑢𝑛𝑢𝑛,>0(2.4) where 𝜙() denotes the 𝑁(0,1) pdf, 𝜔𝑛(>0)is a scale parameter, and 𝜃𝑛(>0) is a shape parameter. When 𝜃𝑛=1, the density becomes the normal pdf with zero mean and standard deviation 𝜔𝑛 (so that when the latter parameter is 1 the pdf collapses to 𝜙(𝑢𝑛)). Values of 𝜃𝑛 above (below) unity correspond to densities skewed to the right (left). Let 𝐔 be an N-dimensional random vector of independent tpn components 𝑢𝑛 with zero mode and unitary scale 𝜔𝑛=1. Its pdf is𝑓𝐔(𝐮𝜽)=𝑁𝑛=1𝑓𝑈𝑛𝑢𝑛1,𝜃𝑛,(2.5) where 𝑓𝑈𝑛() is as in (2.4) (with 𝜔𝑛=1) and 𝜽=[𝜃1𝜃𝑁]. An N-dimensional random vector 𝐗 is said to be 𝐹𝑆-𝑆𝑁𝑁(𝝁,𝐀,𝜽) distributed if there is a random vector 𝐔 with density (2.5) and two vectors 𝝁 (the joint mode) and 𝜽 (the “shape vector”) and a nonsingular matrix 𝐀 (the “scale matrix”) such that 𝐗=𝝁+𝐀𝐔. Vector 𝐗has pdf𝑓𝐗||||(𝐱𝝁,𝐀,𝜽)=det(𝐀)1𝑓𝐔𝐀1(𝐱𝝁)𝜽.(2.6) It is straightforward to confirm that (i) when 𝜽=𝟎, this density collapses to the pdf of a 𝑁𝑁(𝝁,𝐀𝐀) distribution, (ii) the 𝐹𝑆-𝑆𝑁𝑁(𝝁,𝐀,𝜽) distribution is unimodal with mode 𝝁, invariant with respect to 𝐀 and 𝜽, and (iii) by construction, the FS-SN class is closed under nonsingular affine transformations.

3. The Marginal FS-SN Distributions

To establish additional notations, let 𝐈𝑁 denote the identity matrix of order N, and let 𝜂(𝐳) the number of zero elements in vector 𝐳, 𝜓(𝐳) one if all elements of vector 𝐳 are nonnegative and zero otherwise, and 𝐤(𝑖)=(𝑘1(𝑖),,𝑘𝑛(𝑖),,𝑘𝑁(𝑖)) the generic element of the Nth Cartesian power of {1;1}(withcardinal2𝑁), 𝐊(𝑖)=diag𝑛(𝑘𝑛(𝑖))(𝑁×𝑁), Θ(𝑖)=diag𝑛(𝜃𝑘𝑛𝑛(𝑖))(𝑁×𝑁), Ω(𝑖)=[𝐀Θ(𝑖)𝐊(𝑖)][𝐀Θ(𝑖)𝐊(𝑖)]=𝐀Θ2(𝑖)𝐀, 𝝎(𝑖)=[diag(Ω(𝑖))]1/2, 𝝎(𝑖)=𝝎(𝑖)𝜾𝑁, Δ(𝑖)=𝝎1(𝑖)𝐀Θ(𝑖)𝐊(𝑖) and Ω(𝑖)=𝝎1(𝑖)Ω(𝑖)𝝎1(𝑖)=Δ(𝑖)Δ(𝑖).

Proposition 3.1. The pdf and the cdf of the N-dimensional random vector 𝐗𝐹𝑆-𝑆𝑁𝑁(𝝁,𝐀,𝜽)(3.1) with nonsingular scale matrix 𝐀  can be expressed, respectively, as 𝑓𝐗(𝐱𝝁,𝐀,𝜽)=2𝑁𝑖=1𝑁𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1𝑔𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀,𝐹(𝑖)𝐗(𝐱𝝁,𝐀,𝜽)=2𝑁𝑖=1𝑁𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1𝐺𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀,(𝑖)(3.2) where 𝑔𝐗() and 𝐺𝐗() are pdfs and cdfs of singular 𝑆𝑈𝑁𝑁,𝑁(𝝁,𝟎,𝝎(𝑖),Ω(𝑖)) distributions, with Ω(𝑖)=𝐈𝑁Δ(𝑖)Δ(𝑖)Ω(𝑖)=𝐈𝑁Δ(𝑖)[𝐈𝑁Δ(𝑖)].  The latter functions may be written as 𝑔𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀(𝑖)=2𝑁𝜂(𝐱𝝁)𝜑𝑁(𝐱𝝁𝛀(𝑖))𝜓𝐊(𝑖)𝚯1(𝑖)𝐀1,𝐺(𝐱𝝁)𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀(𝑖)=2𝑁𝚽2𝑁𝟎𝝎1(𝑖)(𝐱𝝁)𝛀(𝑖)=2𝑁{𝐳𝐳𝟎,𝐀𝚯(𝑖)𝐊(𝑖)𝐳𝐱𝝁}𝜑𝑁𝐳𝐈𝑁𝐝𝐳.(3.3)

Note that2𝑁𝑖=1𝑁𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1=𝑁𝑛=1𝜃𝑛+𝜃𝑛121𝑁𝑖=1𝑁𝑛=1𝜃𝑘𝑛𝑛(𝑖)=1.(3.4) Hence, the distribution 𝐹𝑆-𝑆𝑁𝑁 can be envisaged as a finite mixture of singular 𝑆𝑈𝑁𝑁,𝑁 distributions.

As pointed out by Arellano-Valle and Azzalini [14, Appendix C], the rank deficiency of Ω(𝑖)does not affect the properties of the SUN distributions and its only impact is of a computational nature. In our case, it actually simplifies the computation of the pdf values because the evaluation of a normal cdf is not required anymore, unlike when computing (2.1), the general expression of a SUN pdf.

In order to derive the marginal pdfs and cdfs of 𝐗, one needs to consider its partition 𝐗=[𝐗𝟏𝐗𝟐]with 𝐗1 and 𝐗2 of dimensions 𝑁1 and 𝑁2, respectively, and the corresponding partitions𝝁𝝁=1𝝁2𝐀,𝐀=1𝐀2𝚫,𝚫(𝑖)=1𝚫(𝑖)2(𝛀𝑖),𝛀(𝑖)=11(𝑖)𝛀12𝛀(𝑖)12(𝑖)𝛀22(,𝝎𝑖)𝝎(𝑖)=1(𝑖)𝟎𝟎𝝎2,(𝑖)𝝎(𝑖)=𝝎1(𝑖)𝝎2(𝑖)(3.5) with 𝐀1(𝑁1×𝑁), Δ1(𝑖)=𝝎11(𝑖)𝐀1Θ(𝑖)𝐊(𝑖)(𝑁1×𝑁), Ω11(𝑖)=𝐀1Θ2(𝑖)𝐀1(𝑁1×𝑁1), 𝝎1(𝑖)=[diag(Ω11(𝑖))]1/2, Ω11(𝑖)=𝝎11(𝑖)Ω11(𝑖)𝝎11(𝑖)=Δ1(𝑖)Δ1(𝑖), and 𝝎1(𝑖)=𝝎1(𝑖)𝜾𝑁1. Proposition 3.2 follows directly from Proposition 3.1 and from the result of Arellano-Valle and Azzalini [14, Appendix A] on the marginal distributions of members of the SUN class.

Proposition 3.2. Let 𝐗=[𝐗1𝐗2]𝐹𝑆-𝑆𝑁𝑁(𝝁,𝐀,𝜽). Then, the marginal pdf and the cdf of the 𝑁1-dimensional subvector 𝐗1are, respectively, 𝑓𝐗1𝐱1𝝁1,𝐀1=,𝜽2𝑁𝑖=1𝑁𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1𝑔𝐗1𝐱1𝝁1,𝟎,𝝎1(𝑖),𝛀11,𝐹(𝑖)𝐗1𝐱1𝝁1,𝐀1=,𝜽2𝑁𝑖=1𝑁𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1𝐺𝐗1𝐱1𝝁1,𝟎,𝝎1(𝑖),𝛀11,(𝑖)(3.6) where 𝑔𝐗1() and 𝐺𝐗1() are pdfs and cdfs of singular 𝑆𝑈𝑁𝑁1,𝑁(𝝁1,𝟎,𝝎1(𝑖),Ω11(𝑖)) distributions, with Ω11(𝑖)=𝐈𝑁Δ1(𝑖)Δ1(𝑖)Ω11(𝑖)=𝐈𝑁Δ1(𝑖)[𝐈𝑁Δ1(𝑖)]. The latter functions may be written as 𝑔𝐗1𝐱1𝝁1,𝟎,𝝎1(𝑖),𝛀11(𝑖)=2𝑁𝜂(𝐱1𝝁1)𝜑𝑁1𝐱1𝝁1𝛀11𝜓𝐊(𝑖)(𝑖)𝚯(𝑖)𝐀1𝐀1𝚯2(𝑖)𝐀11𝐱1𝝁1,𝐺𝐗1𝐱1𝝁1,𝟎,𝝎1(𝑖),𝛀11(𝑖)=2𝑁Φ𝑁+𝑁1𝟎𝝎11(𝐱𝑖)1𝝁1𝛀11(𝑖)=2𝑁{𝐳𝐳𝟎,𝐀1𝚯(𝑖)𝐊(𝑖)𝐳𝐱1𝝁1}𝜑𝑁𝐳𝐈𝑁𝐝𝐳.(3.7)

Appendix

Proof of Proposition 3.1

When 𝜔𝑛=1, the pdf of the univariate tpn (2.4) can be written as𝑓𝑈𝑛𝑢𝑛1,𝜃𝑛=1+𝜃2𝑛1𝑢𝑛𝜃𝑛1+1+𝜃𝑛21𝑢𝑛𝜃𝑛,(A.1) where𝜎(𝑧𝜎)=0(𝑧<0),2𝜋12(𝑧=0),𝜎𝜙𝑧𝜎(𝑧>0).(A.2) Hence, from (2.5),𝑓𝐔(𝐮𝜽)=𝑁𝑛=11+𝜃2𝑛1𝑢𝑛𝜃𝑛1+1+𝜃𝑛21𝑢𝑛𝜃𝑛=2𝑁𝑁𝑖=1𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1𝑘𝑛(𝑖)𝑢𝑛𝜃𝑘𝑛𝑛(𝑖).(A.3) Note that (𝑘𝑛(𝑖)𝑢𝑛𝜃𝑘𝑛𝑛(𝑖))=0 whenever 𝑘𝑛(𝑖)𝑢𝑛<0. Hence, the nonzero terms in the latter summation are those associated with N-tuples 𝐤(𝑖) for which 𝑘𝑛(𝑖)𝑢𝑛0(𝑛=1,,𝑁). If 𝑢𝑛0(𝑛=1,,𝑁) there is only one such term. If 𝐮 includes 𝜂(𝐮) zero elements, there are 2𝜂(𝐮) nonzero identical terms in the previous summation. In both cases, the density of 𝐔 may be expressed as follows:𝑓𝐔(𝐮𝜽)=2𝑁𝑁𝑛=1𝜃𝑛+𝜃𝑛11𝜑𝜃sgn(𝑢𝑛)𝑛𝑢𝑛=𝑁𝑛=1𝜃𝑛+𝜃𝑛11lim𝑁𝜆+𝑛=1𝜃2𝜑𝑛𝑢𝑛Φ𝜆𝜃𝑛𝑢𝑛𝜃+2𝜑𝑛1𝑢𝑛Φ𝜆𝜃𝑛1𝑢𝑛=𝑁𝑛=1𝜃𝑛+𝜃𝑛11lim𝑁𝜆+𝑛=1𝜃𝑛1𝑠𝑢𝑛0,𝜃𝑛2,𝜆+𝜃𝑛𝑠𝑢𝑛0,𝜃2𝑛=,𝜆𝑁𝑛=1𝜃𝑛+𝜃𝑛11lim2𝜆+𝑁𝑖=1𝑁𝑛=1𝜃𝑘𝑛𝑛(𝑖)𝑠𝑢𝑛0,𝜃2𝑘𝑛𝑛(𝑖),𝑘𝑛(𝑖)𝜆=2𝑁𝑁𝑛=1𝜃𝑛+𝜃𝑛121𝑁𝑖=1𝜑𝑁𝚯1(𝑖)𝐮𝐈𝑁lim𝜆+Φ𝑁𝜆𝐊(𝑖)𝚯1(𝑖)𝐮𝐈𝑁,(A.4) where sgn() is the sign function and 𝑠(𝑣0,𝜎2,𝛼) is the pdf of the univariate SN distribution with zero location parameter, scale parameter 𝜎, and shape parameter 𝛼:𝑠𝑣0,𝜎2=2,𝛼𝜎𝜑𝑣𝜎Φ𝛼𝑣𝜎.(A.5)

From the above expression of 𝑓𝐔(𝐮𝜽), by considering the change of variable 𝐗=𝝁+𝐀𝐔 with 𝐀 nonsingular, one obtains the pdf of 𝐗:𝑓𝐗(𝐱𝝁,𝐀,𝜽)=2𝑁𝑁𝑛=1𝜃𝑛+𝜃𝑛121𝑁𝑖=1𝜑𝑁(𝐱𝝁𝛀(𝑖))×lim𝜆+Φ𝑁𝜆𝐊(𝑖)𝚯1(𝑖)𝐀1(𝐱𝝁)𝐈𝑁𝑁𝑛=1𝜃𝑘𝑛𝑛(𝑖)=2𝑁𝑖=1𝑁𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1(𝐱)(A.6) with(𝐱)=2𝑁𝜑𝑁(𝐱𝝁𝛀(𝑖))lim𝜆+Φ𝑁𝜆𝐊(𝑖)𝚯1(𝑖)𝐀1(𝐱𝝁)𝐈𝑁.(A.7) In order to show that (𝐱) is the pdf of a 𝑆𝑈𝑁𝑁,𝑁(𝝁,𝟎,𝝎(𝑖),Ω(𝜆,𝑖)), note that(𝐱)=2𝑁𝜑𝑁(𝐱𝝁𝛀(𝑖))lim𝜆+Φ𝑁𝜆1+𝜆2𝚫(𝑖)𝛀1(𝑖)𝝎11(𝑖)(𝐱𝝁)1+𝜆2𝐈𝑁=𝜑𝑁×(𝐱𝝁𝛀(𝑖))lim𝜆+Φ𝑁𝜆/1+𝜆2𝚫(𝑖)𝛀1(𝑖)𝝎1(𝑖)(𝐱𝝁)𝐈𝑁𝜆2/1+𝜆2𝚫(𝑖)𝛀1(𝑖)𝚫(𝑖)Φ𝑁𝟎𝐈𝑁=lim𝜆+𝑔𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀,(𝜆,𝑖)(A.8) where 𝑔𝐗() is the density of a 𝑆𝑈𝑁𝑁,𝑁(𝝁,𝟎,𝝎(𝑖),Ω(𝜆,𝑖)) distribution with𝛀𝐈(𝜆,𝑖)=𝑁𝜆1+𝜆2𝚫(𝑖)𝜆1+𝜆2𝚫(𝑖)𝛀(𝑖).(A.9) Thus, as lim𝜆+Ω(𝜆,𝑖)=Ω(𝑖),lim𝜆+𝑔𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀(𝜆,𝑖)=𝑔𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀(𝑖).(A.10) The simplified expression for 𝑔𝐗(𝐱𝝁,𝟎,𝝎(𝑖),Ω(𝑖)) presented in Proposition 3.1 is obtained from (A) simply by taking into account thatlim𝜆+Φ𝑁𝜆𝐊(𝑖)𝚯1(𝑖)𝐀1(𝐱𝝁)𝐈𝑁=2𝜂(𝐱𝝁)𝜓𝐊(𝑖)𝚯1(𝑖)𝐀1(𝐱𝝁).(A.11) As regards the cdf of 𝐗,𝐹𝐗(𝐱𝝁,𝐀,𝜽)=𝑧𝑥𝑓𝐗(=𝐳𝝁,𝐀,𝜽)𝐝𝐳2𝑁𝑖=1𝑁𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1𝑧𝑥𝑔𝐗𝐳𝝁,𝟎,𝝎(𝑖),𝛀=(𝑖)𝐝𝐳2𝑁𝑖=1𝑁𝑛=11+𝜃2𝑘𝑛𝑛(𝑖)1𝐺𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀.(𝑖)(A.12) Moreover, one gets from(2.1)𝐺𝐗𝐱𝝁,𝟎,𝝎(𝑖),𝛀=Φ(𝑖)2𝑁𝟎𝝎1(𝑖)(𝐱𝝁)𝛀(𝑖)Φ𝑁𝟎𝐈𝑁=2𝑁Φ2𝑁𝟎𝝎1(𝑖)(𝐱𝝁)𝛀(𝑖)=2𝑁{𝐳𝐳𝟎,𝐀𝚯(𝑖)𝐊(𝑖)𝐳𝐱𝝁}𝜑𝑁𝐳𝐈𝑁𝐝𝐳.(A.13) The latter equality follows from the singularity of Ω(𝑖), which for given 𝐱 allows one to write the probability of𝟎𝝎𝐫1(𝑖)(𝐱𝝁),(A.14) where 𝐫𝑁(𝟎,Ω(𝑖)), as the probability of𝐈𝑁𝟎𝝎𝚫(𝑖)𝐳1(𝑖)(𝐱𝝁){𝐳𝐳𝟎,𝐀𝚯(𝑖)𝐊(𝑖)𝐳𝐱𝝁}(A.15) for 𝐳𝑁(𝟎,𝐈𝑁).