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TESTING FOR STRUCTURAL CHANGE IN THE PRESENCE OF AUXILIARY MODELS

Published online by Cambridge University Press:  01 December 2004

Eric Ghysels
Affiliation:
University of North Carolina and CIRANO
Alain Guay
Affiliation:
Université du Québec à Montréal, CIRPÉE, and CIREQ
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Abstract

Several estimation procedures such as the efficient method of moments (EMM) of Gallant and Tauchen (1996, Econometric Theory 12, 657–681) and indirect inference procedure of Gouriéroux, Monfort, and Renault (1993, Journal of Applied Econometrics 8, S85–S118) involve two models, an auxiliary one and a model of interest. The role played by both models poses challenges and provides new opportunities for hypothesis testing beyond the usual Wald-, Lagrange multiplier–, and likelihood ratio–type tests. In this paper we present and derive the asymptotic distribution theory for various classes of tests for structural change. Some procedures are extensions of standard tests, whereas others are specific to the dual model setup and exploit its unique features.The first author gratefully acknowledges financial support from Fonds pour la Formation de Chercheurs et l'aide à la Recherche (FCAR). The second author acknowledges the financial support of the Natural Sciences and Engineering Research Council of Canada through a grant to NCM2 (Network for Computing and Mathematical Modeling). We also thank Alastair Hall and Éric Renault for comments on an earlier draft of the paper.

Type
Research Article
Copyright
© 2004 Cambridge University Press

1. INTRODUCTION

There is now a fully developed asymptotic distribution theory for various types of test statistics associated with generalized method of moments (GMM) and simulated method of moments (SMM) estimators. The seminal paper by Hansen (1982) on GMM proposes a widely used test for overidentifying restrictions, and Gallant (1987) and Newey and West (1988) present generic Wald-Lagrange multiplier (LM)–, and likelihood ratio (LR)–type tests. Andrews and Ploberger (1994) deal with optimal tests when a nuisance parameter is present only under the alternative. One of the most prominent applications of such test statistics involves the hypothesis of structural change with unknown breakpoint.1

It should be noted that various tests for the structural change hypothesis were developed for the GMM estimator; see, e.g., Andrews and Fair (1988), Dufour, Ghysels, and Hall (1994), Ghysels et al. (1997), Ghysels and Hall (1990), Guay (2003), Hall and Sen (1999), Hoffman and Pagan (1989), and Sowell (1996a), among others.

McFadden (1989), Pakes and Pollard (1989), and Duffie and Singleton (1993) extend the GMM framework to estimation methods involving simulated moments. A comprehensive treatment of Wald-, LM-, and LR-type tests for SMM can be found in Gouriéroux, Monfort, and Renault (1993). Ghysels and Guay (2003) derive optimal structural change tests with unknown breakpoint for SMM.

In recent years a number of estimation procedures have been proposed that involve a dual model setup. Examples include asymptotic least squares (ALS) of Gouriéroux, Monfort, and Trognon (1985), the indirect inference (II) method of Gouriéroux et al. (1993), and the efficient method of moments (EMM) procedure of Gallant and Tauchen (1996). Estimation procedures involving auxiliary models are more commonly used, particularly in situations where likelihood-based estimation or method of moments is infeasible. Many empirical examples can be found in macroeconomic and financial econometrics literature. These procedures are driven by the fundamental distinction between an auxiliary model, parameterized by a vector θ, and a model of interest, which is parameterized by ρ. The distinct role played by both models can be viewed as adding complications to the formulation of traditional tests and can also be viewed as the basis for formulating new classes of tests. The purpose of our paper is to examine both issues.

We present several classes of tests for structural change; some are extensions of tests proposed for GMM and SMM whereas others genuinely exploit features unique to the dual model setup. We proceed in two steps. First we ignore the simulation uncertainty and deal with tests for structural change in a GMM-type setup involving an auxiliary model. Such tests are based on the ALS principle. Next we add the simulation uncertainty and present a generic class of tests for structural change with unknown breakpoints for EMM and II estimators. Although Ghysels and Guay (2003) deal with structural change tests for SMM, they do not consider estimation methods involving an auxiliary model, such as ALS, II, and EMM.

Among the tests for structural change specifically tailored for EMM and II is a class of tests based on a principle of simulated scores that is specific to the combination of an auxiliary model and simulation-based estimation. The simulated score tests we propose use simulated series from a restricted null model of interest. Using the reprojection arguments of Gallant and Tauchen (1998) we can fit a sieve semi-nonparametric (SNP) density to the simulated data. Under the null the simulated data should yield a reprojection score generator that is a martingale difference sequence when applied to the actual sample data.

Our analysis also relates to a EMM diagnostic test proposed by Liu and Zhang (1998). Their test, although meant to be a simulated score test, is closely related to one of the structural change tests we propose. We generalize and extend the test Liu and Zhang (1998) suggest. Recent work by van der Sluis (1998) also proposes structural change tests for EMM. We show that the asymptotic derivations in van der Sluis are invalid for the proposed statistics and compare our tests with the Hansen J-type and Hall–Sen-type tests discussed in van der Sluis (1998).

The paper is organized as follows. In Section 2 we discuss tests for structural change with unknown breakpoint. Section 3 deals with simulated score tests. Section 4 covers nonnested hypothesis testing, and Section 5 concludes.

2. MODELS AND PARAMETER ESTIMATORS

In this section we describe the data generating processes and the various classes of estimators we will consider. Section 2.1 is devoted to the description of the data generating processes. Section 2.2 covers the parameter estimators.

2.1. The Data Generating Processes

The data generating process is described by a parametric nonlinear simultaneous equations model, namely:

where

corresponds to the vector of dependent variables, whereas {xt} is the vector of exogenous variables. Both vector processes are stationary and observable; in addition {xt} is a homogeneous Markov process independent of {εt} and {ut}. The latter two are latent processes with εt white noise with known distribution G0.

2

The assumption of white noise can be relaxed; see Gouriéroux et al. (1993) for further discussion.

The fact that only one lag is considered in (2.1) and (2.2) is not essential and can easily be relaxed.3

In principle an infinite number of lags can be considered, though at a cost of additional regularity conditions, as discussed by Gallant and Tauchen (1996).

It will also be convenient to define the vector Zt−1 ≡ (yt−1,xt). Equations (2.1) and (2.2) correspond to the data generating processes considered by Gouriéroux et al. (1993), Gallant and Tauchen (1996), and Dridi, Guay, and Renault (2003). Because we will be dealing with simulation-based estimators we assume that samples of simulated {yts(ρ)}t=1T can be generated uniquely through (2.1) and (2.2), given ρ and conditional on initial values u0 and y0 and on the observed path of exogenous variables {xt}t=1T. Throughout the paper we assume that all processes are stationary under the null of no structural change. Following Andrews and McDermott (1995), one can extend the asymptotic distribution of the estimators and corresponding test statistics to nonlinear models with deterministically trending variables. As Andrews and McDermott show, this would only involve some straightforward modifications to the estimation of covariance matrices.

The indirect inference method of Gouriéroux et al. (1993) and the efficient method of moments of Gallant and Tauchen (1996) are estimation procedures designed for situations where the log-likelihood function of the structural model

is computationally intractable and where {p(yt|Zt−1,ρ)}t=1T is a sequence of time-invariant conditional densities. The likelihood-based method is therefore replaced by an instrumental criterion that involves a vector of parameters θ ∈ Θ ⊂ Rq, namely:

Minimizing (2.4) yields an M-estimator

for θ. The auxiliary model parameters θ and those of the structural model are related through a system of G-equations:

where ρ0 is the true value of ρ defined for the structural model (2.1) and (2.2) and θ*, called the pseudo-true value, is the value that minimizes the limit (as T → ∞) of the M-estimation criterion (2.4). Equation (2.5) yields a so-called binding function θ* = b0). The II and EMM procedures provide, in different ways, simulation-based approximations to the binding function. Moreover, the function in (2.5) must satisfy the following assumption.

Assumption 2.1. For the purpose of identification, pGq in (2.5), where

are both of full column rank.

Finally, it will be useful to split the parameter vector ρ into two subvectors ρ = (ρ12). There are at least two motivating reasons for this. First, following Andrews (1993) one can consider tests for partial structural change where only a subvector ρ1 of the parameter vector of interest ρ is tested for structural change. Second, following Dridi and Renault (2001) and Dridi et al. (2003) one can also consider situations where only a subvector ρ1 of ρ is of direct interest, whereas ρ2 consists of nuisance parameters, such as parameters pertaining to distributional assumptions. Such a situation, which Dridi and Renault (2001) and Dridi et al. (2003) label semiparametric II, also suggests tests for structural change for subvectors corresponding to parameters of economic interest. Throughout the remainder of this paper we will discuss the implications of partial structural change and semiparametric II. To keep the notational complexity minimal, we avoid splitting the parameter vector ρ into subvectors. All the results we present can easily be modified to take into account the special cases of testing the null hypothesis of structural change for subvectors.

2.2. Parameter Estimators

The ALS estimator of Gouriéroux, Monfort, and Trognon (1985) is a procedure for estimating ρ through an auxiliary model parameterized by θ. Its main advantage, which we exploit here for expository purpose, is that it does not involve simulation uncertainty. Sidestepping this source of uncertainty, at least at a first stage, allows us to focus first and foremost on the key issue of testing for structural change when an auxiliary model is present.

2.2.1. The Asymptotic Least Squares Estimator.

We will consider several ALS estimators. In particular, we define the estimator for the entire sample of the parameter vector of the auxiliary model as the following M-estimator:

where θ ∈ Θ ⊂ Rq. Some tests for structural change involve parameter estimators over subsamples. We will call full sample estimators, such as (2.6), restricted estimators because the parameters are assumed identical across subsamples. To define an unrestricted estimator we consider explicitly two subsamples: the first is based on observations t = 1,…,[Tπ] , and the second subsample covers t = [Tπ] + 1,…,T where π ∈ Π ⊂ (0,1). The separation [Tπ] represents a possible breakpoint, and [·] denotes the greatest integer function. The unrestricted ALS estimators for the first and the second subsamples are

The unrestricted least squares estimators of the parameter vector ρ for the first and second subsamples are obtained by

where WiT(π) are positive definite matrices, g is defined in (2.5), and i = 1,2 corresponding to the appropriate subsample. The restricted ALS estimator for ρ is obtained via a function relating θ* to the parameter of interest. This function is defined as g(θ*,ρ0) = 0 where

replaces θ*, i.e., the estimator that minimizes as T → ∞ the limit of the M-criterion. Hence, the restricted (i.e., full sample) estimator is

where WT is a G × G positive definite matrix.

2.2.2. The Indirect Inference Estimator.

The II method of Gouriéroux et al. (1993) also involves the binding function that relates the estimator for the auxiliary model to the estimator of the structural model θ* = b0). The binding function is unknown, however, and therefore is approximated by simulation. Assume one selects a value of ρ and, using equations (2.1) and (2.2), one simulates the process {yts(ρ)}t=1T. The estimator of the auxiliary model is then defined as

where Z0s are the initial values (y−1,x0) for the s simulated path. Note also that Zt−1s(ρ) ≡ (yt−1s(ρ),xt). For S simulated paths, we construct

, where

is a consistent estimator of the binding function. The indirect estimator of ρ is obtained as the solution of the following minimum distance problem:

where WT is a q × q positive definite matrix.

For certain structural change tests we will need again to define subsample estimators. They are obtained with the auxiliary model for the first and the second subsamples, namely:

and

Therefore the indirect estimators for the first and the second subsamples are obtained by

where i = 1,2 and WiT(π) are positive definite matrices.

To conclude this section we elaborate on the simulation of processes with structural breaks. Suppose the parameters of interest for the two subsamples are ρi for i = 1,2. Then for the first subsample one generates data based on (2.1) and (2.2), modified accordingly, namely, r(yts,yt−1s,xt,ut1) = 0 and q(uts,ut−1sts1) = 0 for t = 1,…,[Tπ]. This is repeated for the second subsample, which covers t = [Tπ] + 1,…,T with ρ2 as parameter. Hence, one creates a series {yts12)}t=1T ≡ ({yts1)}t=1[Tπ], {yts2)}t=[Tπ]+1T).

2.2.3. The Efficient Method of Moments Estimator.

According to the data generation processes (2.1) and (2.2), Gallant and Tauchen (1996) define what they call the maintained model via the corresponding sequence of time-invariant densities

, whereas the auxiliary model is represented by a sequence of time-invariant densities {f1(Z0|θ), f (yt|Zt−1,θ)}t=1, θ ∈ Θ ⊂ Rq. It should be noted that we continue to use Zt−1 as the conditional information set. Typically, Gallant and Tauchen consider densities conditional on yt−1. However, in some circumstances Zt−1 contains only xt, as, e.g., is the case with reprojection schemes (see Gallant and Tauchen, 1998). For the sake of simplicity we will keep the conditioning set as Zt−1, and it will be obvious from the context what the conditional information set is. The following assumption introduced by Gallant and Tauchen (1996) is used for the validity of the EMM criterion as a specification test for the maintained model.

Assumption 2.2. The maintained model

is smoothly embedded within the auxiliary model {f (Z0|θ),f (yt|Zt−1,θ)}t=1 θ ∈ Θ; i.e., for some open neighborhood

, it is such that p(yt|Zt−1,ρ) = f [yt|Zt−1,b(ρ)],t = 1,2,… for every

and p(Z0|ρ) = f (Z0|b(ρ)) for every

.

Under this embedding assumption, the parameters of the auxiliary model (θ*) are related to the parameters of the maintained model (ρ0) according to θ* = b0). Assumption 2.2 is comparable to Assumption 2.1; both play the same role guaranteeing identification of ρ via the auxiliary model. However, Assumption 2.2 is stronger than Assumption 2.1. Indeed, under Assumption 2.2 the EMM estimator is fully efficient.

The EMM estimator is obtained in two steps. The first step is to compute the (pseudo) maximum likelihood estimate of the auxiliary model:

and the corresponding estimate of the information matrix:4

See Gallant and Tauchen (1996) for alternative consistent estimators of I.

In the second step, a vector of moment conditions is constructed using the expectation under the maintained model of the scores from the auxiliary model. The EMM estimator is obtained by minimizing a GMM criterion function formed by the preceding moment conditions, i.e.,

where

and yts(ρ),Zt−1s(ρ)t=1TS is a long series of realizations simulated from the maintained model with the parameter vector ρ. Under suitable regularity conditions discussed in Gallant and Tauchen (1996) and Assumption 2.2, we have

where Mρ = (∂/∂ρ′)m0,θ*) and I is the outer product of scores, as suggested by the estimator in (2.17). All these results apply to the case where the number of simulations goes to infinity. In the case of possible structural changes with unknown breakpoint, theoretical results based on the number of simulations equal to infinity are not so appealing, as the computational cost involved can be prohibitively high. For this reason, the asymptotic results need to be modified to account for a finite number of simulations. When S is finite, the randomness of the EMM estimator

will depend not only on the randomness of

but also on the randomness of the moment conditions due to a finite length of series simulated from the structural model. Therefore the asymptotic variance-covariance matrix in equation (2.17) is scaled by (1 + 1/S) using arguments similar to those of Duffie and Singleton (1993).

To conclude this section we present partial sample estimators that appear in certain tests for structural change. The unrestricted EMM estimator for the subsamples are defined as

where

is the estimator of the matrix I for the ith subsample, and

The simulation of processes when a break is present can be characterized by the following sequence of densities: {p(Z01),p(yt|Zt−11)}t=1[TSπ] for the first subsample and {p(yt|Zt−12)}t=[TSπ]+1TS for the second. It is important to note that the simulated path length is a function of the fraction of the sample (π). This point is crucial. Indeed, the asymptotic distribution of several structural change tests could depend on the nuisance parameter S, and hence the critical values could depend on S, in the case where the simulated path length is not split according to the presumed breakpoint π. Section 3.2 will examine this problem.

3. GMM-LIKE TESTS FOR STRUCTURAL CHANGE WITH UNKNOWN BREAKPOINT

The purpose of this section is to generalize GMM-based tests for structural change presented by Andrews (1993), Andrews and Ploberger (1994), Sowell (1996a, 1996b), and Ghysels, Guay, and Hall (1997). A variety of tests are proposed, ranging from (optimal) Wald-, LM-, and LR-type tests to predictive tests with unknown breakpoint. In this section we deal with the issues posed by procedures involving two models, an auxiliary one and a model of interest. We note that the role played by both models poses challenges and provides new opportunities for hypothesis testing. Here we only deal with the usual Wald-, LM-, and LR-type and predictive tests. In the next section we cover tests that are specifically designed for the dual model setup. We cover tests based on ALS, II, and EMM estimators. One of the first issues to resolve is to clearly define the null hypothesis of interest in tests for structural change analysis. The analysis in Section 3.1 involves the ALS because it allows us again to focus directly on the key issues of hypotheses and test statistics. The added complication of simulation uncertainty is considered in Section 3.2.

3.1. Tests for Asymptotic Least Squares

The purpose of this section is twofold: (1) clearly spell out the null hypotheses involved in tests for structural change when an auxiliary model is present and (2) adapt the usual Wald-, LM-, and LR-type and predictive tests for such situations. A section is devoted to each of the two issues.

3.1.1. The Null Hypotheses.

The null hypothesis of interest for structural parameters is

The fact that we estimate the parameter vector ρ indirectly via an auxiliary model implies that we also should consider the null hypothesis

The null hypotheses (3.1) and (3.2), although related, are obviously not identical. Accepting H0θ implies that there is no structural change for ρ because of the identification Assumption 2.1 for the binding function. Rejecting H0θ does not necessarily imply that H0ρ is violated because the dimension of θ is equal or greater than the dimension of ρ. To unravel whether the rejection of H0θ is due to a structural change of the overidentifying restrictions, one can follow the approach of Sowell (1996b) and characterize via projection the subspace that identifies ρ. Such projection can distinguish structural change of the structural parameters from breaks in the overidentifying restrictions. This distinction becomes even more interesting when we allow for partial structural change, i.e., when we consider subvectors of ρ. In particular, in the context of semiparametric II, following Dridi et al. (2003), this may involve a subvector of nuissance parameters ρ2 for which structural change may be more tolerated.

To elaborate further on the distinction between the null hypotheses (3.1) and (3.2), and in particular the interpretation of rejecting the null hypotheses, we consider a sequence of local of alternatives:

where h(η,ν,π), for π ∈ [0,1] , is a q-dimensional function that can be expressed as the uniform limit of step functions, η ∈ Ri, ν ∈ Rj such that 0 < ν1 < ν2 < ··· < νj < 1 and θ* is in the interior of Θ. The function h(·) allows for a wide range of alternative hypotheses (see Sowell, 1996b). The parameter ν locates structural changes as a fraction of the sample size, and the vector η defines the local alternatives. To simplify the notation h(η,ν,(t/T)) will be denoted h(ν). The following theorem provides the asymptotic distribution for the optimally weighted g(·) for both subsamples, using WT = ΩT−1,5

This expression may exist only with probability going to one. When this expression is singular, a g-inverse can be used in place of the inverse (see Andrews, 1993). Similar comments apply elsewhere.

where ΩT is the full sample estimator of the optimal weighting matrix Ω that is defined in Appendix E.

THEOREM 3.1. Under Assumptions 2.1, A.1, and B.1 and sequence of local alternatives (3.3), we have

where

is a G-dimensional vector of independent Brownian motions.

Proof. See Appendix E.

Under the null hypothesis (3.2), a version of Corollary 1 of Sowell (1996a) holds; namely, there exists an orthonormal matrix C such that

where BBp(π) is a p-dimensional Brownian bridge, BGp(π) is a Gp-dimensional Brownian motion, C is such that Ω−1/2Gρ(Gρ′Ω−1Gρ)−1 × Gρ′Ω−1/2 = C′ΛC,CC′ = Id where Id is the identity matrix, and

For the function g(·) evaluated at the estimator obtained from the second subsample, we have

where BBG(π) is defined previously and BGp*(π) = BGp(1) − BGp(π).

As shown by Sowell (1996b), structural change tests can be constructed in projecting on the appropriate subspace. The limiting stochastic processes in (3.4) and (3.5) are equivalent to the limiting stochastic processes for the GMM estimator in Sowell or those obtained for the SMM estimator in Ghysels and Guay (2003). Under the null hypotheses (3.1) and (3.2), the results in (3.4) and (3.5) show that the limiting continuous stochastic processes are linear combinations of p Brownian bridges, one for each parameter estimated, and Gp Brownian motions, spanning the space of overidentifying restrictions, where G is the dimension of g(·).

We can refine now the null hypothesis (3.1). In particular, following Hall and Sen (1999) we consider the generic null, for the case of a single breakpoint, that separates the identifying restrictions across the two subsamples:

where PG = Ω−1/2Gρ(Gρ′Ω−1Gρ)−1Gρ′Ω−1/2. Moreover, the overidentifying restrictions are stable if they hold before and after the breakpoint. This is formally stated as H0Og(π) = H0Og1(π) ∩ H0Og2(π) with

Using the projection applied to the decomposition appearing in (3.4) and (3.5), it is clear that instability must be reflected in a violation of at least one of the three hypotheses: H0Iρ(π), H0Og1(π), or H0Og2(π). It is only the former of those three that corresponds to the null hypothesis (3.1). Violation of H0Og1(π) or H0Og2(π) means that there are reasons to reject the null hypothesis H0θ in (3.2) but still accept H0ρ in (3.1). Various tests can be constructed with local power properties against any particular one of these null hypotheses (and typically no power against the other two).

To conclude we need to discuss the implication of various structural change tests in the presence of auxiliary models. The decomposition of the hypothesis (and associated tests) into H0Iρ(π), H0Og1(π), or H0Og2(π) has different implications for the structural model. The auxiliary model can be viewed as a window through which information is obtained about the structural model. Consequently, structural change can only be assessed via the information about the structural model revealed by the auxiliary model. For example, Guay and Renault (2003) examine indirect encompassing when both models are misspecified and estimated by auxiliary models. In the first step of their proposed procedure, the auxiliary model is used only to obtain consistent estimators of structural model parameters. Structural parameter instability detected through the intermediary of the auxiliary model is crucial for the consistency of the procedure. However, instability of the overidentifying restrictions (of the auxiliary model) without change of the structural parameters is innocuous.

3.1.2. Test Statistics.

A structural change test is obtained for the vector of parameters ρ when the function ΩT−1/2g(·) is projected on the subspace identifying the parameters with the first subsample estimator

. This statistic is

where Gρ,T is a consistent estimator of Gρ. The statistic with the estimator of the second subsample is

A structural change test for overidentifying restrictions is obtained when projecting the function ΩT−1/2g(·) on the subspace orthogonal to the subspace identifying the parameters. For example, the statistic with the first subsample estimator is

In the case of unknown breakpoint, statistics can be constructed by mapping on π ∈ Π. Andrews and Ploberger (1994) in the context of maximum likelihood estimation and Sowell (1996a, 1996b) for GMM estimation derive optimal tests that are characterized by an average exponential mapping. In the case of a one-time structural break alternative and a particular integral weight function for h(·) in (3.3), the tests with the greatest weighted average asymptotic power have the following form for structural parameter instability:

where R(π) is the weight function over the set of possible breakpoints Π. The parameter c controls the distance of the alternative. For close alternatives c → 0, the asymptotic test with the greatest weighted average power is an average (ave) over π ∈ Π and has the form ∫QiT(π) dR(π). For a distant alternative c → ∞, the functional is log ∫ exp(½QiT(π)) dR(π). The supremum form supπ∈Π Qit(π) often used in the literature corresponds to the case where c/(1 + c) → ∞. The LM (or LMT(π) for given π) test statistic of structural change corresponds to the case where R(π) = 1/(π(1 − π)) dπ. A Wald (WaldT(π)) and an LR-type (LRT(π)) test statistic can be constructed as usual with the restricted and unrestricted ALS estimators. Following Andrews (1993), we can show that WaldT(π) = LMT(π) + op(1) and LRT(π) = LMT(π) + op(1).

The following proposition gives the asymptotic distribution for the exponential mapping for QiT when QiT corresponds to the Wald-, LM-, and LR-ratio-type tests.

PROPOSITION 3.1. Under the null hypothesis H0 in (3.1) and Assumptions 2.1, A.1, and B.1, the following processes indexed by π for a given set Π whose closure lies in (0,1) satisfy

This result is obtained through the application of the continuous mapping theorem (see Pollard, 1984). The asymptotic distribution is a quadratic form of weighted Brownian bridge such as when the breakpoint is known the asymptotic distribution is a chi-square with a degree of freedom equal to the dimension of the structural vector parameters. In the case of an unknown breakpoint, critical values are given in Andrews (1993) for a weighting equal to 1/(π(1 − π)).

The next proposition gives the asymptotic distribution for the exponential mapping for QiT0 when QiT0 is the statistic for the structural change in overidentifying restrictions corresponding to the null H0Ogi(π).

PROPOSITION 3.2. Under the null hypothesis of no structural change for the overidentifying restrictions and Assumptions 2.1, A.1, and B.1, the following processes indexed by π for a given set Π whose closure lies in (0,1) satisfy

with Q1,Gp(π) = BGp(π)′BGp(π) and Q2,Gp(π) = BGp*(π)′BGp*(π), where BGp(π) is a Gp-dimensional vector of independent Brownian motion, BGp*(π) = BGp(1) − BGp(π), and i = 1,2.

The asymptotic distribution is a quadratic form of Brownian motion such as when the breakpoint is known the asymptotic distribution is a chi-square with a degree of freedom equal to Gp. Critical values for Q1,Gp(π) and Q2,Gp(π) with respective weighting equal to 1/π and 1/(π(1 − π)) are tabulated in Guay (2003). Predictive tests, discussed in Ghysels et al. (1997) and Guay (2003), can also be constructed, and the asymptotic distribution of those tests can be easily obtained from Theorem 3.1.

3.2. Structural Change for II and EMM

The analysis in Section 3.1 involves the ALS estimator of Gouriéroux et al. (1985), a procedure that we have chosen to discuss first as it features the estimation of ρ through an auxiliary model parameterized by θ. We now turn our attention to procedures with similar features but that require simulations to obtain the binding function appearing in (2.5). Sidestepping simulation uncertainty allowed us to focus exclusively on the key issue of testing for structural change when an auxiliary model is present. The results in Ghysels and Guay (2003) may help us to understand the effect of simulation uncertainty on tests for structural change. Ghysels and Guay propose a set of tests for structural change in models estimates via SMM (see Duffie and Singleton, 1993) and show that the number of simulations does not affect the asymptotic distribution or the asymptotic local power of tests for structural change. Hence, the asymptotic results obtained for GMM-based tests are also valid for SMM-based procedures. The intuition for this result is that in the case of tests for structural change one compares parameter estimates that are subject to the same simulation uncertainty (unlike tests of a fixed hypothesis where the distance of the estimates to the null depends on the simulation uncertainty). Ghysels and Guay (2003) show that the asymptotic distribution under the local alternatives depends on the number of simulations. Nonetheless, they also show by a Monte Carlo investigation that a relatively small number of simulations suffices to obtain tests with desirable small sample size and power properties.

The purpose of this section is to extend the results of Ghysels and Guay (2003). In particular, it will be shown that for both the II and EMM estimators, the simulation uncertainty does not affect the asymptotic distribution of tests for structural stability. Hence, there is an asymptotic analogue between ALS-based tests and II- or EMM-based procedures. We begin with the II procedure to show that this is indeed the case.

THEOREM 3.2. For the full and the partial sample II estimators appearing in (2.13) and (2.14), under Assumptions 2.1, A.1, and C.1 and sequence of local alternatives (3.3), we have

and for the second subsample

where

are two q-dimensional vectors of mutually independent Brownian motions, and ΩT is a consistent estimator of Ω = J−1IJ−1.

Proof. See Appendix E.

Under the null hypothesis, by replacing ΩT by

in the expressions of Theorem 3.2, a version of Corollary 1 of Sowell (1996a) can be easily shown such as

For the second subsample, we have

where Bqp*(π) = Bqp(1) − Bqp(π). To obtain these results, we note that

is a q-dimensional vector of standard Brownian motion. As shown in Section 3.1.2, structural change tests can be constructed by projection on the appropriate subspace. A structural change test is obtained for the vector of parameters ρ when the difference between the estimator obtained with the auxiliary model for the data and the average estimators obtained with simulated paths is projected on the subspace identifying the parameters for the first or the second subsample. The statistic based on the first subsample estimator is

where bρ,T is a consistent estimator of bρ0).6

See Gouriéroux et al. (1993).

A structural change test for overidentifying restrictions is obtained by projecting the same function on the subspace orthogonal to the subspace identifying the parameters. The resulting statistic based on the first subsample estimator is

The asymptotic distribution under the null of the exponential mappings of these statistics is given in Proposition 3.1 for the parameter stability and in Proposition 3.2 for stability of overidentifying restrictions.

Using Theorem 3.2, we show that simulation uncertainty does not affect the asymptotic distribution of tests for structural stability under the null. Hence, the implication of structural change detected in the auxiliary model has the same interpretation as in the ALS case. In Section 3.1.1 it was noted that the importance of instability in the auxiliary model for the structural model depends on which hypothesis is violated, namely, H0Iρ(π), H0Og1(π), or H0Og2(π). An interesting case to examine can be found in the work of Dridi and Renault (2001), who develop a generalization of II to semiparametric settings. Their approach produces a theory of robust estimation despite misspecifications of the structural model. Suppose economic theory only provides information about a subvector of parameters of interest ρ1 (in our notation) and direct estimation of the structural model cannot be performed so that the econometrician relies on II. To simulate the structural model, an additional nuisance parameter vector ρ2 is required. Because we are only interested in a consistent estimator for ρ1, the importance of finding structural change in the auxiliary model depends on the impact of instability on the parameter vector of interest. In particular, instability for the nuisance parameters ρ2 or for overidentifying restrictions without affecting stability of the parameter vector of interest has no impact on the consistency of the semiparametric II estimator. Structural change tests must therefore focus on the parameter vector of interest ρ1. With our results, partial structural stability tests for this parameter vector of interest can be constructed, and the asymptotic distribution of exponential mappings is given in Section 3.1.2.

Next, we turn to the EMM estimator, in particular the theorem that follows.

THEOREM 3.3. For the partial sample EMM estimators appearing in (2.18), (2.23), and (2.24), under Assumptions A.1, C.1, and D.1 and sequence of the local alternatives (3.3), we have

and for the second subsample

where

are two q-dimensional vectors of mutually independent Brownian motions.

Proof. See Appendix E.

Structural change tests can be constructed by replacing IT by

as shown in the previous sections. These statistics based on the first subsample estimator are

where Mρ,T is a consistent estimator of Mρ.

The asymptotic distribution of the resulting tests is the same as the one derived earlier if we note that

is a q-dimensional vector of Brownian motions. The asymptotic distributions under the null are then given in Proposition 3.1 for the parameter stability and in Proposition 3.2 for stability of overidentifying restrictions.

van der Sluis (1998) proposes similar structural change tests for EMM. However, in contrast to our strategy, the length of the simulated series used to construct the structural change tests in van der Sluis (1998) is the same for the estimation of the full sample estimator of ρ and for the evaluation of the moment restrictions with the unrestricted estimators

. Such a strategy has an important impact on the asymptotic distribution as will be shown in the remainder of this section. Suppose that the length of the simulated series is equal to TS. The statistic proposed by van der Sluis is based on the following moment restrictions:

for i = 1,2. For the case where the moment restrictions are evaluated at

, which is also obtained with a simulated path equal to TS, we can show the following result under the null:

The LM structural change statistic is constructed by projecting the preceding moment restrictions on the subspace identifying the parameters. Such a statistic has the usual asymptotic distribution (see Proposition 3.1). This result holds because the nuisance term introduced by simulation

cancels out. However, the asymptotic distribution of a structural change test for overidentifying restrictions constructed by projection on the subspace orthogonal to the subspace identifying the parameters is not the same as given in Proposition 3.2. In this case, one can show that the asymptotic distribution is a function of the following process:

The quadratic form of Brownian motion given in Proposition 3.2 is augmented by an extra term. This extra term contains a nuisance parameter that depends on the length of the simulated path, and hence the critical values depend on S. Consequently, the statistics in van der Sluis (1998) are valid only in the case where S equals infinity or would require critical values that need to be computed for various values of S (the applications in van der Sluis, 1998, use S = 3 with S = ∞ critical values).

4. TESTS EXPLOITING AUXILIARY MODELS

Thus far we examined a set of tests that were introduced to the literature in the context of GMM and SMM estimation and have their roots in the earlier literature (for references, see, e.g., Andrews, 1993). We studied the consequences of having estimation and inference via auxiliary models. The purpose of this section is to present statistics that are designed to test for structural breaks and take advantage of the dual model setup. We cover two types of tests. A first class relates to recent work of Liu and Zhang (1998) on diagnostic testing of EMM score generators, which we show are implicitly tests for structural change. The second class is based on the simulated score principle.

4.1. The Liu and Zhang Tests

The results obtained in Appendix E allow us to examine the specification test in the EMM framework proposed by Liu and Zhang (1998). This test is a measure of the overall goodness of fit of the auxiliary model. The zeta statistic introduced by Liu and Zhang is defined as follows:

where

. We will see that the zeta statistic is in fact a structural change statistic test for the parameters of the auxiliary model. Using results derived in this paper, we can show that the asymptotic distribution of the zeta statistic under the alternative is given by

where BB(π) is a vector of an independent Brownian bridge of dimension q. The second term in the bracket shows that the zeta statistic is powerful against a structural change alternative for the parameter vector θ. However, this test is not an optimal test of structural change as defined by Andrews and Ploberger (1994) and Sowell (1996a, 1996b).

4.2. Simulated Score Tests

We introduce specific structural change tests for EMM called simulated score tests. The tests rely on simulated series from a restricted null model of interest. Using the reprojection arguments of Gallant and Tauchen (1998), we can fit a sieve SNP density to the simulated data. Under the null, the simulated data should yield a reprojection score generator that is a martingale difference sequence when applied to the actual sample data.

In the case of structural change tests, the simulated score test consists of evaluating the score for the actual sample data for a possible breakpoint using the estimator of the auxiliary model for the simulated data. The first step is to simulate series with the restricted estimator defined in equation (2.18). The second step is to obtain the estimator of θ of the auxiliary model with the simulated series. The score for this second step is

where N is the length of the simulated series. The third step is to evaluate the score with the data for a possible breakpoint at the estimator obtained in the second step. The simulated score structural change test is then based on the following statistic:

where

is the estimator of the auxiliary model obtained with simulated series. The next theorem gives the asymptotic distribution of the statistic defined previously.

THEOREM 4.1. Under Assumptions A.1, C.1, and D.1 and the alternative (3.3)

where

are two q-dimensional vectors of mutually independent Brownian motions.

Proof. See Appendix E.

Under the null, the asymptotic distribution differs from the one obtained in Theorem 3.3. In particular, it depends on the length of the simulated series N. However, replacing N by TSπ for π ∈ Π as the length of the simulated series results in the asymptotic distribution appearing in Theorem 3.3. This is the same argument as the one developed in the discussion of the van der Sluis statistic. Using TSπ as the length for the simulated series yields asymptotic distributions under the null and under the local alternative that are identical to the distributions of the test proposed in Section 3.2. Structural change tests can then be constructed by replacing IT by ĨT = (1 + 1/S)IT as shown in the previous sections. The asymptotic distributions of these structural change tests are given in Proposition 3.1 for the parameter stability and in Proposition 3.2 for the stability of overidentifying restrictions. Hence, the simulated score tests have the same asymptotic distribution under the null and the alternative as the tests appearing in Section 3.2. However, the small sample properties can differ. In particular, the usual statistics proposed in Section 3.2 are based on the unrestricted estimators θiT for i = 1,2. For small or large values of π ∈ Π, the properties of the unrestricted estimators

could be poor because the partial samples used to obtain these estimators are relatively small. This problem does not occur for the computation of the simulated score test.

5. CONCLUSIONS

Estimation procedures involving auxiliary models are more commonly used, particularly in situations where likelihood-based estimation is infeasible. Many empirical examples can be found in the financial econometrics literature, particularly pertaining to the estimation of continuous time processes. Financial markets experience regular disruptions, sometimes modeled as so-called jumps. There may be more fundamental shifts at work, and the tests proposed here would be applicable.

Besides generalizing existing test procedures we also introduced new ones that rely on the dual model setup. The simulated score tests introduced in the paper can easily be extended to hypotheses other than structural breaks. As a by-product of the paper, we also showed that some recently proposed diagnostic tests for auxiliary models are de facto tests for structural change, albeit suboptimal ones.

APPENDIX A: TECHNICAL ASSUMPTIONS

To simplify the notation, ψt(yt|Zt−1,xt;θ) will be denoted as ψt(θ).

A.1. General Assumptions.

Assumption A.1. Let us make the following assumptions:

APPENDIX B: ASYMPTOTIC LEAST SQUARES REGULARITY CONDITIONS

Assumption B.1. The following are assumed to hold:

APPENDIX C: INDIRECT INFERENCE REGULARITY CONDITIONS

To simplify the notation, ψ(yts(ρ)|Zt−1(ρ),θ) will be denoted as ψts(θ(ρ)).

Assumption C.1. The following are assumed to hold:

APPENDIX D: EFFICIENT METHOD OF MOMENTS REGULARITY CONDITIONS

To simplify the notation (∂/∂θ)log[f (yts(ρ)|Zt−1s(ρ),θ)] will be denoted as (∂/∂θ)log[fts(θ(ρ))].

Assumption D.1. The following are assumed to hold:

APPENDIX E: PROOF OF THEOREMS

E.1. Proof of Theorem 3.1.

We need to use the following lemma to prove the theorem.

LEMMA E.1. Under Assumptions 2.1, A.1, and B.1 and the alternative hypothesis (3.3), the asymptotic distribution of the full sample ALS estimator is

and the asymptotic distributions of the unrestricted M-estimators are

Proof of Lemma E.1. First, the asymptotic distribution for the restricted estimator is shown. By the mean value expansion for the first-order condition evaluated at

:

where

for some 0 ≤ λ(k) ≤ 1 and k = 1,…,q. Because

is consistent for

, and by Assumption A.1, the preceding expression yields

By Assumption A.1, we also have

where

. The asymptotic distribution of the full sample estimator

is then given by

The mean value expansion for the restricted ALS estimator is

where

for some 0 ≤ λ(k) ≤ 1, k = 1,…,p, and

is defined previously.

By the fact that the first term of the right-hand side is equal to zero, the full sample estimator

is only a function of the asymptotic distribution of

. Because

is consistent for θ*, then

, and because

is consistent for ρ0, then

. Under Assumptions 2.1, A.1, and B.1, the continuous mapping theorem, and the consistency of

, the preceding expression yields

and by the result (E.1),

The optimal estimator is obtained with the following weighting matrix (this expression may exist only with probability → 1; when this expression is singular, a g-inverse can be used in place of the inverse):

where

is consistent estimator of I. (In pure time series context, a consistent estimator can be obtained using methods developed by Gallant (1987), Andrews and Monahan (1992), and Newey and West (1994), among others. In the general case, the same methods apply, but the score must be centered around its empirical mean (see Gouriéroux et al., 1993).)

Now we derive the asymptotic distribution for the unrestricted estimators. By the mean value expansion for the M-estimators

for the first subsample

where

for some 0 ≤ λ(k) ≤ 1 and k = 1,…,q. Because

is consistent for

, and under Assumption A.1, this yields

By the mean value expansion for the M-estimators

for the second subsample

where

for some 0 ≤ λ(k) ≤ 1 and k = 1,…,q. By Assumption A.1,

using

. Because

is consistent for

, we then obtain

By the weak convergence of the score (Assumption A.1), we get

The asymptotic distributions of the unrestricted M-estimators are then given by

Proof of Theorem 3.1. First, we show the result for the first subsample. We do the mean value expansion for

, which yields

where

are defined previously. By using Lemma E.1 and under Assumptions 2.1, A.1, and B.1 with the convergence in probability of ΩT to Ω and the continuous mapping theorem, we obtain that

Because Ω−1/2Gθ J−1I1/2B(π) is a q-dimensional standard Brownian motion, the result follows. The asymptotic distribution for the second sample can be obtained in a similar way. █

E.2. Proof of Theorem 3.2.

LEMMA E.2. Under Assumptions 2.1, A.1, and C.1 and the alternative (3.3), the asymptotic distribution of the II estimator is

and the asymptotic distributions of the unrestricted simulated M-estimators are

Proof of Lemma E.2. Now, we derive the asymptotic distribution of the restricted estimator

. For the simulated path s, we have the following mean value expansion for the first-order condition evaluated at

:

where

for some 0 ≤ λ(k) ≤ 1 and k = 1,…,q and θ* = b0). Under Assumption C.1 and by the consistency of

,

The asymptotic distribution of

is then given by

In contrast to the asymptotic distribution of the estimator

obtained with data, the asymptotic distribution of

does not depend on the alternative for obvious reasons. The mean value expansion for the restricted II estimator is

where

is defined as in the proof of Lemma E.1 but for the estimator obtained with S simulated paths. By Assumption C.1 and the consistency of

, this yields

Using results (E.1) and (E.3), the asymptotic distribution of

is given by

The asymptotic distribution depends on the matrix W0 and the number of simulations S. The restricted optimal II estimator is obtained with the following weighting matrix:

. (See Gouriéroux et al., 1993.)

Now, we derive the asymptotic distribution for the unrestricted estimators. The mean value expansion of the M-estimators for the first subsample evaluated at

gives

where

for some 0 ≤ λ(k) ≤ 1 and k = 1,…,q and θ* = b0). This yields the following expression:

We can obtain the equivalent expression for

by a similar mean value expansion.

By Assumption C.1, we have the following weak convergence of the score for the first and the second subsamples:

Given the preceding results, the asymptotic distributions of the unrestricted simulated M-estimators are, respectively:

Proof of Theorem 3.2. By a mean value expansion for the first subsample, we have that

By Lemmas E.1 and E.2, Assumption C.1, and the consistency of

, we obtain that

Because Ω−1/2J−1I1/2B(π) is a q-dimensional vector of standard Brownian motions, the result follows. The asymptotic distribution for the second sample is obtained similarly. █

E.3. Proof of Theorems 3.3 and 4.1.

LEMMA E.3. Under Assumptions A.1, C.1, and D.1 and the alternative hypothesis (3.3), the asymptotic distribution of the full sample EMM estimator is

Proof of Lemma E.3. First, the asymptotic distribution for the restricted estimator is shown. By the mean value expansion for the first-order condition evaluated at

where

for some 0 ≤ λ(k) ≤ 1 and k = 1,…,q. By Assumption A.1 and the consistency

, the preceding expression yields

where

. By the last Assumption of A.1 and noting that ψt(·) = −log ft(·), the asymptotic distribution of the score at the pseudo-true value θ* is

The asymptotic distribution of the full sample estimator

is then given by

The mean value expansion of the first-order condition evaluated at the unrestricted EMM estimator is

where

for some 0 ≤ λ(k) ≤ 1 and k = 1,…,p and

is defined previously.

Under Assumptions A.1 and D.1 and the consistency of

, this yields

because

converge in probability to −J. Now we examine the expression mTS0,θ*). By definition

Using the last assumption of C.1 with ψt(·) = −log ft(·), we obtain

By (E.5) and (E.6), the asymptotic distribution of

is then given by

In the case where S = ∞, the term B(1)s disappears. █

Proof of Theorem 3.3. First, we show the result for the first subsample. We do the mean value expansion for

, which gives

with

for some

is defined previously. Let us examine the expression m1S0,θ*). By definition

Using the last assumption of C.1 with ψt(·) = −log ft(·), this yields

By using Lemmas E.1 and E.3, Assumptions A.1 and D.1, the result (E.7), and the consistency of

, we get

The asymptotic distribution for the second sample can be obtained in a similar way. █

Proof of Theorem 4.1. First, we show the asymptotic distribution of the estimator

obtained with the simulated series for ρ fixed at the restricted estimator

. The mean value expansion of the score of the auxiliary model evaluated at

is given by

with

for some 0 ≤ λ(k) ≤ 1 and k = 1,…,q, θ* = b0), and

defined previously. By the asymptotic distribution of the restricted estimator

given in Lemma E.3, Assumptions A.1 and D.1, result (E.6), and the consistency of

, we obtain that

The mean value expansion of the score evaluated at

for the data under the alternative for the first subsample is

with obvious notation for

. By definition

and using the last assumption of A.1 with ψt(·) = −log ft(·), this yields

By the asymptotic distribution of the

derived previously, Assumptions A.1 and D.1, result (E.9), and the consistency of

, we obtain under the alternative that

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