Volume 17, Issue 3 pp. 338-372
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Point-optimal panel unit root tests with serially correlated errors

Hyungsik Roger Moon

Hyungsik Roger Moon

Department of Economics, University of Southern California, Los Angeles, CA, 90089 USA

Department of Economics, Yonsei University, Seoul, Korea

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Benoit Perron

Benoit Perron

Universite de Montreal, CIREQ, CIRANO, C.P. 6128, Succ. centre-ville, Montreal, QC H3C 3J7, Canada

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Peter C. B. Phillips

Peter C. B. Phillips

Cowles Foundation, Yale University, PO Box 208281 New Haven, CT 06520-8281, USA

Department of Economics, University of Auckland, Owen G. Glenn Building, Private Bag 92019, Auckland 1142, New Zealand

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First published: 01 April 2014
Citations: 13

Summary

Generalizations of the point-optimal panel unit root tests of Moon, Perron and Phillips (MPP) are developed to cover cases of serially correlated errors. The resulting statistics involve two modifications relative to those of MPP: (a) the error variance is replaced by the long-run variance; (b) centring of the statistic is adjusted to correct for second-order bias effects induced by the correlation between the error and lagged dependent variable.

1. Introduction

There has been much recent interest in testing for the presence of stochastic trends in large panels; see, e.g., Breitung and Pesaran (2008) and Breitung and Westerlund (2013). A prototypical model consists of a deterministic trend component urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0001 and an (unobserved) stochastic component urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0002 for some observable panel observations urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0003 for individual urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0004 in period urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0005 satisfying
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0006(1.1)
where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0007 is an error term that has zero mean and is stationary over time, and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0008 for simplicity. Dynamic panel models with incidental trend components of this type arise in many applications in microeconometrics, multicountry growth studies and international finance. Empirical interest often centres on the individual dynamics and on whether there is commonality and persistence across individuals (i.e. that the autoregressive parameters urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0009 are all unity) or whether such commonality occurs for certain subgroups of individuals.
Moon et al. (2007, hereafter MPP) developed tests that are point optimal against a specific alternative hypothesis. MPP adopted a local-alternative set-up, specifying the autoregressive parameter as lying in a local vicinity of unity whose width narrows as the sample size increases, according to the form
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0010(1.2)
where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0011 is a sequence of i.i.d. random variables and κ is a parameter defining the width of the vicinity as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0012. The null hypothesis of interest is then
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0013(1.3)
with the alternative
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0014(1.4)

The MPP tests are point optimal in the sense of giving highest power against a specific set of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0015. These tests were derived under the assumption that the error term urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0016 is independent across individual units and over time. They represent a panel extension of the work of Elliott et al. (1996) in the time-series case where the autoregressive parameter converges to unity at a rate of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0017, regardless of the deterministic component in the model.

Independence assumptions are not realistic in many empirical applications and in this work we extend the MPP tests by allowing for serially correlated errors urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0018. In their Section 6.4 (p. 436), MPP briefly mentioned this extension. Here, we provide explicit test statistics that have optimal asymptotic properties. The modified tests replace estimated variances of the errors in MPP with estimated long-run variances, and adjust centring terms. Our main purpose is to provide the form of the modified tests and to give their asymptotic properties so that they can be used in empirical work.

The paper is organized as follows. In Section 2., we show how to construct the tests, give results for cases with no fixed effects, fixed effects and incidental trends, and discuss implementation. In Section 3., we report some simulation findings. We conclude in Section 4, and in the Appendix we provide technical derivations and supporting lemmata.

2. Tests under Serial Correlation

Following MPP, in the following analysis, we consider three deterministic trend cases: (a) no individual effects (i.e. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0019 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0020); (b) fixed effects (i.e. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0021); (c) heterogeneous or incidental linear trends (i.e. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0022). In each case, we proceed in three steps. First, we define the likelihood ratio (urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0023) statistic under Gaussianity, which is known to be optimal by the Neyman–Pearson lemma when the null and alternative hypotheses are simple. Then, we show that this statistic can be approximated by a simpler version with parameters that are consistently estimable. Finally, we derive the asymptotic distribution of this approximation (with appropriate recentring). In all three cases, this asymptotic distribution coincides with the one in MPP.

Our notation is similar to that of MPP. Denote by Z, D, Y, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0024 and U the urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0025 observation matrices whose urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0026th elements are urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0027, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0028, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0029, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0030 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0031, respectively. Define the urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0032 vectors urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0033, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0034 and set urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0035, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0036. Define urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0037, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0038 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0039, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0040. Let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0041, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0042, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0043 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0044 denote the transpose of the ith row of Z, Y, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0045 and U, respectively. With this notation, the model has the matrix form
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0046
where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0047.

Define urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0048, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0049 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0050 as the variance of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0051, the long-run variance of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0052 and the one-sided long-run variance of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0053, respectively, so that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0054. Let Σ, Ω and Λ be the diagonal matrices with elements urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0055, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0056 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0057, respectively. Define urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0058 as the urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0059 covariance matrix of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0060 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0061 as the urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0062 covariance matrix of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0063. As in MPP, we assume that the errors urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0064 are cross-section independent over i.

We assume that the localizing coefficient urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0065 in the local alternative 1.2 is a sequence of i.i.d. random variables with bounded support. Let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0066, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0067 and define the quasi-difference operator
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0068
Set urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0069 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0070.
The quasi-log-likelihood function of the panel Z, which we use in defining the likelihood ratio test statistic, has the form
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0071
for some weight matrix B.

Throughout the paper, we assume panel linear process errors with conditions similar to those in the literature (e.g. Phillips and Moon, 1999). Let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0072, let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0073 be the spectral density of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0074, and let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0075.

Assumption 2.1.(a) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0076, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0077 with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0078 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0079 for some urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0080; (b) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0081 for some urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0082, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0083, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0084, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0085; (c) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0086 and for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0087 and some constant M.

These conditions extend the serial dependence restrictions of Elliott et al. (1996) (e.g. their Condition A) to heterogeneous panels. Assumption 2.1(a) assumes that the error term urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0088 follows a linear process that is heterogeneous across i. The higher moments are needed to ensure the large urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0089 asymptotics of panel data that are heterogeneous across i and serially correlated over t. Under cross-sectional homoscedasticity, these moment conditions could be weakened. Assumptions 2.1(b) and 2.1(c) restrict the temporal dependence of the error term urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0090 to be ‘weak’ uniformly across i. These restrictions exclude long memory type strong dependence. The conditions in Assumption 2.1 are quite weak and are satisfied by many parametric weak dependent processes, such as stationary and invertible ARMA processes.

While Assumption 2.1 is quite general in terms of the serial correlation that is allowed, it is restrictive in that it assumes that all cross-sectional units are independent. This assumption is not reasonable for many interesting empirical data sets, such as cross-country studies where business-cycle effects are likely to induce correlation across countries. As in MPP, we conjecture that the procedures proposed below are valid after appropriate orthogonalization is applied, for example, after the removal of common factors as in Moon and Perron (2004), Bai and Ng (2004) or Phillips and Sul (2003). Moreover, the development of optimal procedures under cross-sectional dependence is beyond the scope of the current paper.

2.1. No fixed effect: urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0091

When urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0092, the model becomes
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0093
Following MPP, in this case we consider local neighbourhoods of unity that shrink at the rate of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0094, so that the rate coefficient urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0095, and one-sided alternatives in which the support of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0096 is a bounded interval urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0097 for some urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0098 so that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0099 under this alternative. In terms of the first moment of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0100, the hypotheses about urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0101 are
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0102(2.1)
and
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0103(2.2)
Suppose that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0104 are Gaussian so that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0105 with known urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0106 and the initial conditions urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0107 are all zeros. By the Neyman–Pearson lemma, rejecting a small value of the log-likelihood ratio test statistic
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0108(2.3)
would be the uniformly most powerful test for the null urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0109 for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0110 against the simple alternative urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0111 for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0112. When the alternative is 1.4 with 2.2, this becomes a point-optimal test.

In order to implement the optimal test statistic 2.3, we need an estimate of the entire urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0113 covariance matrix urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0114. This is a huge high-dimensional covariance estimation problem in a non-parametric set-up. The following theorem provides an approximation of the likelihood ratio test statistic in 2.3 with a statistic where the unknown nuisance parameters are consistently estimable.

Theorem 2.1.Let Assumption 2.1 hold with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0115. Assume that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0116 → 0 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0117. Then, for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0118, we have

urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0119

Note that the approximate likelihood ratio statistic
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0120(2.4)
in Theorem 2.1 employs the Gaussian log-likelihood based on the long-run variance urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0121 with an adjustment of the one-sided long run variance urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0122. The one-sided long-run drift correction appears to be a result of the correlation between the stationary error urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0123 and the lagged dependent variable urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0124. The main advantage of this formulation is that it involves quantities (Ω and Λ) that can be estimated consistently.
The test statistic we propose is to use the approximated log-likelihood ratio 2.4 with appropriate centring. Define
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0125
where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0126 is the sum vector and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0127.

Theorem 2.2.Let Assumption 2.1 hold and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0128 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0129. Then, under the local alternative urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0130, we have

urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0131
where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0132

Remark 2.1.We can interpret the test statistic urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0133as an asymptotic version of the point-optimal test for panel unit roots with possible serial correlation of unknown form in the error term.

Remark 2.2.Compared to the corresponding statistic in MPP, which makes no allowance for serial correlation, there are two differences in urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0134. First, as discussed in MPP, we use the long-run covariance matrix urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0135 instead of the variance matrix urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0136 as the weight matrix. In addition, we recentre the statistic by subtracting the term urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0137, which corrects for the correlation between the stationary error urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0138 and the lagged dependent variable urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0139. This term is not required for the test under temporal independence.

Remark 2.3.The limit distribution of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0140 is the same limit as in MPP (see their Theorem 6).

2.2. Time-invariant fixed effects: urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0141

In this section, we consider the case where the incidental trends urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0142 are fixed over time. This corresponds to the standard fixed effects model. In this case, the model has matrix form
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0143
As before, suppose that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0144 with known urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0145 and the initial conditions urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0146 are all zeros. Then, rejecting a small value of the test statistic,
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0147(2.5)
for the null urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0148 for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0149 and the alternative urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0150 for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0151 is known as the uniformly most powerful invariant test that is invariant with respect to the transformation urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0152 for arbitrary urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0153. Against the alternative in 1.4, this becomes a point-optimal invariant test (e.g. Dufour and King, 1991).

As mentioned in the previous section, this statistic is difficult to implement because of the presence of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0154, the full urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0155 covariance matrix of the error. This again motivates the use of an approximation.

Theorem 2.3.Let Assumption 2.1 hold with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0156 and let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0157 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0158. Then, for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0159, we have

urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0160

Remark 2.4.This approximation is derived under the stronger rate condition urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0161 → 0 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0162 in place of the condition urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0163 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0164 that is used without fixed effects.

Remark 2.5.The approximation involves the same correction for second-order bias as in the case without fixed effects.

Again, the test statistic we propose is the approximate log-likelihood ratio 2.4 with appropriate centring. Define
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0165

Theorem 2.4.Let Assumption 2.1 hold and let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0166 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0167. Then, under the local alternative urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0168, we have

urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0169
where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0170.

This asymptotic distribution is the same as without fixed effects and as in MPP (see their Theorem 9).

2.3. Incidental trends: urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0171

Under heterogeneous linear trends, we follow MPP and use local neighbourhoods of unity that shrink at the slower rate of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0172, so that the rate coefficient is urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0173. The alternative might be two-sided; that is, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0174 with mean urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0175 and variance urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0176, with a support that is a subset of a bounded interval urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0177, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0178, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0179. The slower rate of shrinkage in the local neighbourhoods of unity is the result of the presence of heterogeneous trend effects in the panel. The presence of these incidental trends reduces discriminatory power in testing for the presence of common stochastic trends, so wider localizing intervals are needed to attain non-trivial power functions.

Under these conditions, hypotheses 1.3 and 1.4 can be re-expressed as
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0180(2.6)
and
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0181(2.7)
Again, suppose that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0182 with known urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0183 and the initial conditions urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0184 are all zeros. Then, similar to the case of time-invariant fixed effects, rejecting a small value of the test statistic,
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0185
for the null urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0186 for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0187 and the alternative urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0188 for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0189, is known as the uniformly most powerful invariant test (with respect to the linear transformation urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0190 for arbitrary urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0191), and against the alternative in 1.4, it becomes a point-optimal invariant test. As before, we start by proving the validity of an approximation to this log-likelihood ratio.

Theorem 2.5.Let Assumption 2.1 hold with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0192 and let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0193 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0194. Then, for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0195, we have

urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0196

Remark 2.6.This approximation is derived under the condition urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0197 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0198, which is a stronger rate condition than that used for the intercepts case.

Remark 2.7.As before, the correction is a result of the presence of a second-order bias term arising from the correlation between the lagged dependent variables and the error term.

Again, we propose to use the approximate log-likelihood ratio with appropriate centring as a test statistic. Define
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0199
where
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0200

Theorem 2.6.Let Assumption 2.1 hold and let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0201 as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0202. Then, under the local alternative urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0203, we have

urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0204

As before, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0205 reduces to the statistic from MPP when there is no serial correlation, and it has the same asymptotic distribution as in Theorem 13 of MPP.

2.4. Implementation of the tests

The test statistics urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0206, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0207 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0208 depend on unknown parameters urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0209, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0210 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0211. Let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0212, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0213 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0214 be consistent estimators of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0215, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0216 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0217, respectively. Similarly define the diagonal matrices of these elements as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0218, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0219 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0220. To implement these tests, we can replace Σ, Ω and Λ in urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0221, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0222 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0223 with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0224 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0225 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0226 and we denote the test statistics as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0227, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0228 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0229. We assume the following regarding these estimators.

Assumption 2.2.Under the local alternative, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0230, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0231 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0232.

Remark 2.8.An example of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0233 that satisfies Assumption 2.2 is the time-series sample variance of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0234

urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0235

Remark 2.9.When kernel spectral density estimation is used for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0236 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0237 with bandwidth h, Assumption 2.2 is satisfied if: (a) the kernel function urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0238 is continuous at zero and all but a finite number of other points, satisfying urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0239 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0240 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0241 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0242 for some urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0243 where parameter m is defined in Assumption 2.1(b); (b) the bandwidth h satisfies

urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0244(2.8)
as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0245 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0246; see, e.g., Moon and Perron (2004). If urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0247 for some urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0248 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0249, then the bandwidth condition 2.8 is satisfied if
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0250
that is,
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0251

Theorem 2.7.Under Assumptions 2.1 and 2.2, as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0252 with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0253 we have urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0254, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0255 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0256 under the local alternative.

Implementation of the tests also requires the choice of an alternative to define the likelihood ratio, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0257. MPP have shown that the optimal choice of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0258 is urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0259. With this choice, the likelihood ratio statistics above attain the power envelope. However, this choice is infeasible because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0260 are the parameters under test. MPP proposed the assumption of a common urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0261 for all cross-sectional units, and they called this test a common point-optimal (CPO) test. With this choice, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0262, and we can deduce from Theorems 2.2, 2.4 and 2.6 that under the null hypothesis,
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0263
while under the alternative hypothesis,
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0264

The surprising result here is that neither distribution depends on the choice of c used to construct the test. This feature implies that the power is the same for all choices of c asymptotically, although that choice matters in finite samples. Based on the simulation evidence provided in MPP, we set urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0265 in the simulation below. Of course, this choice of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0266 is not optimal unless the alternative hypothesis is homogeneous (urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0267 for all i) and results in a power loss relative to the power envelope.

3. Monte Carlo simulations

In this section, we report the results of a Monte Carlo experiment designed to assess the finite-sample properties of the tests presented above and compare them with other existing results. For this purpose, we use the same DGP as MPP but employ either an AR(1) or MA(1) process for the innovations. Thus, the generating model has the following form,
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0268
where the innovations follow either an AR(1) process
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0269
or an MA(1) process
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0270
We have also looked at some ARMA(1,1) cases but we do not report those results in order to ease presentation (these results are available from the authors upon request). We consider five specifications for serial correlation: white noise (urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0271), positive AR (urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0272 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0273), negative AR (urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0274 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0275), positive MA (urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0276 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0277) and negative MA (urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0278 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0279).

In all cases, we allow for heterogeneity and draw the idiosyncratic variance urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0280 from a uniform distribution, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0281. This variance is scaled such that the scale of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0282 is the same for all cases. In both the incidental intercepts case urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0283 and the incidental trends case urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0284, the parameters are drawn from urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0285.

We focus the study on the size and size-adjusted power of the CPO test with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0286 for all i, because MPP advocated that choice. For size calculations, we set urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0287 for all i, which corresponds to urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0288 for all i in our local-to-unity framework. For power, we draw urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0289 from a uniform distribution between 0 and 8, as in one of the experiments of MPP. This specification ensures that power should be roughly constant as N and T increase.

We draw comparisons with two existing tests, those of Levin et al. (2002), hereafter LLC, and Im et al. (2003), hereafter IPS. We take three values for n (10, 25 and 100) and two values of T (100 and 250). All tests are conducted at the 5% significance level, and the number of replications is set at 2,000.

Estimation of the long-run variance and one-sided long-run variance is critical to the performance of the CPO test. We estimate these quantities in two ways based on demeaned first differences, as in Remark 2.8. The first method is a non-parametric estimator with quadratic spectral kernel and bandwidth selected in a data-based manner using the Andrews (1991) rule with no pre-whitening (PW). The second method uses pre-whitening where the appropriate model is chosen using BIC among the AR(1), MA(1), ARMA(1,1) and constant-only models. In the case of the LLC test, we follow the recommendation of Levin et al. (2002) and use a Bartlett kernel with a bandwidth equal to urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0290. Westerlund (2009) has shown that this choice gives the LLC test higher power than selecting the bandwidth in a data-dependent way. Similarly, for the IPS and LLC tests, the choice of lag augmentation is critical for performance. We choose this in a data-dependent way by BIC with a maximum of six lags. For both of these tests, we use the finite-sample adjustments provided in the original papers.

The size results are reported in Tables 1 and 3 for the incidental intercepts and trends cases respectively, while size-adjusted power is in Tables 2 and 4. For each of the five serial correlation specifications, each row corresponds to a different test.

Table 1. Size of tests: incidental intercepts
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0291 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0292 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0293
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0294 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0295 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0296
100 250 500 100 250 500 100 250 500
White noise This paper, no PW 1.6 2.2 2.6 2.8 3.2 3.6 4.2 3.7 5.2
This paper, PW 2.4 2.4 2.5 3.0 3.8 4.5 0.6 2.5 4.4
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0297 MPP (2007) 2.9 2.4 2.5 4.8 3.7 4.4 4.3 3.6 4.7
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0298 IPS 6.4 3.7 4.9 7.0 5.2 5.2 8.4 6.9 5.1
LLC 5.8 4.4 4.1 5.8 5.3 3.4 6.0 5.0 3.5
Positive AR This paper, no PW 1.7 1.8 2.9 2.4 2.8 3.3 4.5 4.5 4.9
This paper, PW 2.3 2.1 3.0 1.7 2.3 3.0 0.7 0.4 2.4
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0299 MPP (2007) 0.3 0.5 0.8 0.1 0.1 0.1 0.0 0.0 0.0
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0300 IPS 5.0 4.4 3.6 4.7 3.9 3.5 3.1 3.1 3.5
LLC 5.0 4.2 4.0 4.3 4.3 3.7 2.6 2.8 3.9
Negative AR This paper, no PW 1.7 2.1 2.2 2.5 3.2 4.0 5.4 4.2 5.2
This paper, PW 2.0 2.5 2.1 1.2 2.6 3.3 0.3 1.5 2.2
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0301 MPP (2007) 12.7 13.2 13.6 30.7 30.3 32.4 82.2 81.6 83.9
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0302 IPS 12.8 7.3 5.4 20.4 9.4 7.2 42.6 15.3 9.3
LLC 9.0 5.8 4.2 12.0 7.0 4.0 20.8 8.5 4.3
Positive MA This paper, no PW 1.4 1.7 2.6 2.1 3.0 3.7 4.3 4.5 4.8
This paper, PW 2.5 2.6 3.0 2.7 3.2 4.1 1.6 3.5 4.5
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0303 MPP (2007) 0.7 0.7 0.6 0.3 0.2 0.6 0.0 0.0 0.0
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0304 IPS 6.6 6.1 5.7 6.8 6.4 6.0 7.1 7.4 8.4
LLC 6.1 5.9 4.7 5.4 6.0 4.6 5.2 7.2 5.6
Negative MA This paper, no PW 1.3 2.0 2.6 2.3 3.5 3.6 4.6 4.5 4.3
This paper, PW 1.5 2.4 3.0 0.9 3.1 4.0 0.0 1.6 3.5
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0305 MPP (2007) 17.0 16.7 17.6 40.7 44.1 40.7 93.0 91.8 93.1
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0306 IPS 25.0 13.8 10.2 40.4 22.6 14.3 85.0 50.0 32.9
LLC 15.6 9.4 6.9 22.2 12.3 6.5 56.6 25.9 14.4

Note

  • The table reports the rejection frequency (in %) of a 5% test for a panel unit root. “This paper, no PW” refers to the common point optimal (CPO) tests proposed in this paper with no pre-whitening used when estimating long-run variances and c = 1. “This paper, PW” refers to the CPO tests in this paper with pre-whitening when estimating long-run variances. “MPP (2007)” refers to the CPO tests with c = 1 in MPP that do not allow for serial correlation. “IPS” is the t-bar test of Im et al. (2003) and “LLC” is the test of Levin et al. (2002).
Table 2. Size-adjusted power of tests - Incidental intercepts
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0307 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0308 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0309
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0310 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0311 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0312
100 250 500 100 250 500 100 250 500
White noise This paper, no PW 41.6 49.3 52.9 53.0 62.6 62.8 66.4 75.2 71.7
This paper, PW 43.2 54.8 52.5 45.1 62.2 62.6 40.5 73.0 73.4
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0313 MPP (2007) 50.5 55.1 54.1 59.4 66.4 62.5 76.7 78.7 74.6
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0314 IPS 13.2 18.1 12.9 16.8 17.5 16.9 21.6 18.6 21.3
LLC 3.7 1.9 1.1 5.3 3.3 2.8 5.7 3.8 3.1
Positive AR This paper, no PW 42.9 51.8 45.3 54.8 62.8 63.6 63.7 69.5 73.4
This paper, PW 48.8 53.1 48.0 59.5 64.1 62.2 63.5 73.5 74.8
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0315 MPP (2007) 52.0 54.5 45.4 62.4 60.7 63.9 72.2 73.1 73.7
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0316 IPS 12.0 13.0 16.1 12.4 17.2 14.8 21.3 19.5 20.7
LLC 3.1 2.3 1.8 3.5 2.7 1.6 6.0 5.2 3.5
Negative AR This paper, no PW 42.8 48.3 51.3 53.2 60.3 61.1 63.3 72.0 72.4
This paper, PW 45.0 52.5 51.4 47.2 59.8 61.0 40.0 69.6 76.3
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0317 MPP (2007) 48.4 47.8 50.5 62.9 59.6 60.6 70.1 71.5 74.7
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0318 IPS 13.0 14.6 14.4 19.7 16.1 15.8 22.0 20.0 19.0
LLC 5.2 2.6 1.3 6.1 2.3 2.4 7.9 4.6 3.2
Positive MA This paper, no PW 44.2 48.0 51.3 52.8 63.2 59.8 63.6 72.8 73.0
This paper, PW 47.6 51.8 53.5 59.0 64.5 61.2 58.4 74.7 74.8
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0319 MPP (2007) 52.2 54.0 50.9 61.3 66.4 64.2 72.3 75.8 75.2
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0320 IPS 10.4 12.7 12.1 14.3 16.4 17.4 17.9 20.8 18.7
LLC 2.6 1.9 1.1 4.6 2.7 1.9 5.5 4.0 3.4
Negative MA This paper, no PW 41.4 49.4 47.5 54.8 55.5 59.9 65.9 72.7 77.9
This paper, PW 46.7 51.8 48.7 43.0 57.6 62.2 32.6 68.1 77.8
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0321 MPP (2007) 48.6 48.7 46.3 57.9 57.2 58.4 68.8 70.0 72.1
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0322 IPS 15.0 16.7 14.2 21.2 15.3 18.8 23.9 26.7 22.5
LLC 8.1 2.6 1.6 8.5 4.3 3.7 11.8 6.7 3.6
Table 3. Size of tests: incidental trends
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0323 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0324 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0325
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0326 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0327 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0328
100 250 500 100 250 500 100 250 500
White noise This paper, no PW 0.0 0.1 0.5 0.0 0.6 1.5 0.0 0.5 0.9
This paper, PW 1.0 1.0 1.4 1.8 2.3 2.7 1.4 4.1 4.5
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0329 MPP (2007) 1.7 1.3 1.4 4.6 2.5 2.9 7.2 5.1 4.4
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0330 IPS 8.2 5.5 5.2 10.6 5.6 4.4 14.9 7.5 6.4
LLC 6.4 4.5 2.1 5.8 4.3 1.1 4.8 4.4 0.5
Positive AR This paper, no PW 0.0 0.0 0.5 0.0 0.4 1.5 0.0 0.2 1.2
This paper, PW 0.8 0.4 1.0 1.6 2.2 2.2 2.1 2.1 2.0
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0331 MPP (2007) 0.0 0.0 0.1 0.0 0.0 0.0 0.0 0.0 0.0
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0332 IPS 5.3 3.5 4.4 4.2 3.0 4.0 3.8 2.8 3.3
LLC 3.7 2.7 1.7 2.0 2.6 0.9 0.7 1.2 0.2
Negative AR This paper, no PW 0.0 0.1 0.5 0.0 0.2 1.0 0.0 0.3 1.3
This paper, PW 0.4 0.6 0.7 0.5 1.2 1.9 0.2 1.7 2.1
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0333 MPP (2007) 22.2 19.8 20.3 61.7 58.4 56.8 99.3 99.3 99.1
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0334 IPS 25.3 10.7 7.1 40.6 15.6 8.9 84.1 31.7 13.7
LLC 16.9 7.6 2.8 24.5 9.4 1.6 53.8 14.5 0.5
Positive MA This paper, no PW 0.0 0.2 0.5 0.0 0.6 1.2 0.0 0.2 1.8
This paper, PW 1.0 1.3 1.2 3.7 3.4 2.6 6.5 6.5 5.3
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0335 MPP (2007) 0.1 0.1 0.1 0.1 0.1 0.0 0.0 0.0 0.0
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0336 IPS 8.1 6.6 6.0 10.7 7.2 6.7 12.4 11.4 8.4
LLC 5.5 5.5 1.7 5.6 5.9 1.8 2.6 7.0 0.6
Negative MA This paper, no PW 0.0 0.1 0.4 0.0 0.3 1.1 0.0 0.4 0.9
This paper, PW 0.1 0.7 0.9 0.4 2.4 2.9 0.2 4.0 3.9
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0337 MPP (2007) 31.7 29.1 29.7 77.1 74.8 73.3 100.0 100.0 100.0
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0338 IPS 48.2 23.5 15.3 77.6 42.2 26.6 99.9 86.0 63.0
LLC 38.1 17.7 6.1 61.1 30.1 7.0 96.6 67.8 12.2
Table 4. Size-adjusted power of tests: incidental intercepts
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0339 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0340 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0341
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0342 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0343 urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0344
100 250 500 100 250 500 100 250 500
White noise This paper, no PW 10.8 17.0 15.8 12.9 17.3 17.2 17.5 23.2 26.1
This paper, PW 15.6 17.6 16.2 14.2 20.5 19.3 19.9 27.9 28.2
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0345 MPP (2007) 18.6 19.1 15.6 17.7 20.9 19.4 28.1 27.5 28.9
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0346 IPS 10.5 10.1 10.1 9.8 12.8 12.7 13.9 14.0 11.9
LLC 8.5 6.8 4.9 9.2 7.9 5.1 11.6 8.4 5.8
Positive AR This paper, no PW 11.0 15.6 16.4 10.9 18.1 19.5 18.1 26.0 27.5
This paper, PW 17.1 18.7 16.5 18.8 22.3 19.8 26.2 29.9 29.5
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0347 MPP (2007) 17.7 16.8 15.4 18.7 20.3 19.3 27.6 27.7 28.6
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0348 IPS 8.5 9.9 8.7 11.1 13.5 11.3 12.1 12.6 13.3
LLC 6.2 6.6 3.9 8.5 7.0 6.0 8.6 5.6 5.0
Negative AR This paper, no PW 10.7 15.1 15.2 14.1 16.8 18.0 15.8 23.3 23.8
This paper, PW 13.9 16.6 16.9 16.7 20.1 19.0 20.1 28.6 25.9
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0349 MPP (2007) 16.5 16.6 16.3 21.8 17.5 19.2 26.5 24.3 27.0
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0350 IPS 12.0 9.6 10.4 11.2 9.9 10.9 11.9 10.9 13.8
LLC 10.7 7.3 4.6 10.7 6.1 5.5 11.0 7.5 6.8
Positive MA This paper, no PW 12.0 14.6 18.4 11.9 18.0 22.3 19.3 25.8 30.0
This paper, PW 20.2 17.9 18.3 18.6 21.2 23.8 25.8 30.4 31.0
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0351 MPP (2007) 19.0 16.2 19.3 19.4 20.7 24.4 32.1 28.1 30.3
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0352 IPS 9.1 11.2 10.3 9.9 11.2 11.0 14.0 12.6 16.0
LLC 8.3 7.7 6.0 7.8 8.0 5.1 11.5 7.0 6.9
Negative MA This paper, no PW 10.7 16.3 18.0 13.0 19.3 22.0 15.0 23.2 29.6
This paper, PW 14.3 16.7 17.5 11.8 18.7 20.1 12.2 23.7 29.4
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0353 MPP (2007) 14.0 14.6 16.3 18.1 18.3 21.2 24.1 23.1 27.7
urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0354 IPS 9.9 9.4 10.2 11.2 12.2 11.7 15.5 12.6 14.2
LLC 11.1 6.7 5.2 11.5 8.3 5.5 12.7 7.6 6.9

In general, we see that our CPO test is conservative. This is especially true in the incidental trends case. The test is better behaved without pre-whitening in estimating the long-run variance in the incidental intercepts case, but the reverse is true in the trends case. It is evident that the original MPP test is not robust to the presence of serial correlation with size that can be as low as 0 or as high as 1, and that the extensions proposed here are therefore needed.

Table 2 reports results for size-adjusted power in the intercept case. Size adjustment is needed, given some of the large size distortions reported in Table 1. We see that the size-adjusted power of the CPO tests robust to serial correlation is typically lower than that of uncorrected tests, but the difference becomes smaller as N and T increase, as predicted by theory because the tests have the same asymptotic distribution. Also, we see that these tests have much higher size-adjusted power than either the LLC or IPS tests. The LLC test has poor power because it corrects for bias by adjusting the numerator of the pooled OLS estimator, as pointed out by Moon and Perron (2008) and Breitung and Westerlund (2013).

Table 4 presents size-adjusted power for the incidental trends case. Note that the alternative considered in this scenario is further from the unit root null than in Table 2 because of the different definition of local neighbourhoods. While the CPO tests have lower power in this case, the same conclusions remain as in the intercept case.

4. Conclusion

In this paper we develop generalizations of the point-optimal panel unit root tests of MPP to cover the case where the error term is serially correlated. The resulting statistics have two simple modifications relative to those in MPP. First, the variance of the errors is replaced by the long-run variance. Second, the centring of the statistic is adjusted to accommodate the second-order bias induced by the correlation between the error and lagged values of the dependent variable. Simulations show that these two adjustments lead to appropriately sized tests in most cases.

Acknowledgements

We thank Vanessa Smith for raising with us questions about the performance of the original point-optimal statistics in MPP when there are serial correlated errors and about the need for possibly different correction factors in that case. B. Perron acknowledges financial support from the SSHRC and FQRSC. P. C. B. Phillips acknowledges partial support from the National Science Foundation under Grant Nos. SES-0956687 and SES-1258258.

  1. 1 As mentioned in MPP, the assumption of a bounded support for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0633 is made for convenience, and could be relaxed at the cost of stronger moment conditions. It is also convenient to assume that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0634 are identically distributed, and this assumption could be relaxed as long as cross-sectional averages of the moments urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0635 have well-defined limits.
  2. 2 This assumption of a zero initial value is strong. The treatment of initial values in panel unit root tests is still an open problem. In MPP, we showed that the assumption that the initial observation is drawn from the unconditional distribution cannot be easily extended to the panel case because the resulting test statistic diverges to infinity with probability 1.
  3. 3 Note that Moon and Perron (2008) incorrectly labelled their urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0636 statistic as equivalent to the LLC statistic, while they should have labelled their urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0637 statistic (which has lower power) as equivalent to the LLC statistic.
  4. APPENDIX A:: PROOFS OF THE APPROXIMATIONS IN THEOREMS 2.1, 2.3 AND 2.5

    We provide three appendices. Here, in Appendix A, we provide proofs of Theorems 2.1, 2.3 and 2.5 that approximate the Gaussian log-likelihood ratio statistic. In Appendix B, we provide sketches of the proofs of the limit distribution results in Theorems 2.2, 2.4 and 2.6. In Appendix C, we provide a heuristic proof of Theorem 2.7. We only provide sketches of the proofs in Appendices B and C because the details are similar to those of the corresponding theorems in MPP and can be established with only minor modifications. Throughout the appendices, M denotes a generic (finite) constant.

    Proof of Theorem 2.1.Here, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0355. Let Assumption 2.1 hold and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0356. By definition, we can write

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0357(A.1)
    Write
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0358(A.2)
    where
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0359
    and
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0360(A.3)
    where
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0361
    In the following subsections, we show that under Assumption 2.1, as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0362
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0363(A.4)
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0364(A.5)
    Then, using (A.1)(A.5) with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0365, we deduce that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0366
    as required. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0367

    Proof of Theorem 2.3.Here, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0368. Let Assumption 2.1 hold and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0369. By definition, we have

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0370
    Using (A.2), (A.3), (A.4) and (A.5), we can approximate the first term as
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0371
    Then, the required result for the theorem follows because
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0372(A.6)
    for any urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0373 such that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0374 for some constant M. The proof of (A.6) is available in the following subsection. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0375

    Proof of Theorem 2.5.Here, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0376. Let Assumption 2.1 hold and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0377. By definition, we have

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0378
    Using (A.2), (A.3), (A.4) and (A.5), we can approximate the first term as
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0379
    Also, in the following subsection, we show that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0380(A.7)
    for any urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0381 such that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0382 for some constant M. Then, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0383
    Combining these expressions gives the required result:
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0384

    A.1 Supplementary results

    A.1.1. A useful lemma

    Before we start the proof of (A.4) and (A.5), we introduce a useful technical result. When A is a matrix, we use three different norms, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0385 (where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0386 denotes the maximum eigenvalue), urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0387 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0388 (where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0389 is the urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0390th element of A). It is well known that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0391
    By definition, the covariance matrix of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0392 is urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0393. Let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0394 be the urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0395 matrix whose urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0396 element urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0397 is urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0398 if urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0399 and zero, if urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0400. Let
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0401(A.8)

    Lemma A.1.Let Assumption 2.1 hold. Then, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0402 for some constant M.

    Proof.For the desired result, we show

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0403
    By definition,
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0404
    where the inequality holds because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0405 under Assumption 2.1 and by the triangle inequality.

    First, we show that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0406. Define

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0407
    By adding and subtracting the terms and the triangle inequality, we can bound
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0408
    where
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0409
    For term I1, note that because
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0410
    and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0411, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0412
    where the second inequality uses urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0413, the last inequality uses urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0414 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0415 and the equality uses the Taylor representation of the exponential function. Then,
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0416
    For term I2, note that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0417
    where the first inequality holds because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0418 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0419 and the last inequality holds by the mean-value theorem and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0420. Then,
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0421
    For term I3, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0422
    where the last line holds because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0423. Finally, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0424
    where the second inequality holds because
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0425
    By combining terms urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0426, we have the required result
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0427
    The proof of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0428 follows in a similar fashion and is omitted. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0429

    Proof of (A.5).We prove the required result when urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0430 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0431. Because

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0432
    the required result follows if we show
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0433(A.9)
    and
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0434(A.10)

    For A.9, we follow similar arguments used in proving urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0435 on p. 831 (in the proof of Lemma A2) of Elliott et al. (1996), and have for some constant M

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0436
    where the second inequality holds because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0437 and by Lemma A.1, and the last inequality holds because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0438

    For A.10, we also follow similar arguments to those used in proving urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0439 on p. 831 (in the proof of Lemma A2) of Elliott et al. (1996), and have for some constant M

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0440

    Proof of (A.4).We prove the required result when urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0441 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0442. By replacing urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0443 in urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0444 with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0445, we can decompose urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0446 as

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0447
    where
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0448
    and
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0449
    First, similar arguments to those in the proof of (A.5) lead to
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0450
    Then, the required result follows if
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0451
    which follows if
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0452
    Note that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0453
    Using similar arguments to those used for the proof of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0454, we can show that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0455
    For urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0456, we show
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0457(A.11)
    Because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0458, the desired result follows. Because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0459, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0460
    Because trurn:x-wiley:13684221:media:ectj12030:ectj12030-math-0461, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0462
    For term I, we can bound
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0463
    Then, for some constant urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0464, we can bound
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0465
    as required. Next,
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0466
    and, by Assumption 2.1(c),
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0467
    because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0468, as required. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0469

    A.1.2. More preliminary results

    In this section, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0470 and let Assumption 2.1 hold. Define urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0471 to be the urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0472 matrix whose urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0473th element is urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0474, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0475 is defined in Assumption 2.1.

    Define urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0476. Direct calculations show that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0477
    and
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0478(A.12)
    Define
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0479
    where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0480 is the tth element of the vector x and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0481

    Lemma A.2.(a) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0482 for all k; (b) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0483 for some finite constant M.

    Proof.Part (a). By definition, for urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0484

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0485
    For urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0486, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0487
    as required.

    Part (b). By definition,

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0488
    as required. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0489

    Lemma A.3.Suppose that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0490 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0491 are urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0492 vectors such that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0493 is bounded, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0494 is the (t)th element of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0495. Then, (a) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0496; (b) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0497, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0498 is defined in A.8.

    Proof.Part (a). The proof is similar to that of Lemma A1 of Elliott et al. (1996) and is omitted.

    Part (b). We replace urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0499 in the proof of Lemma A.1 with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0500. Then, the required result follows if we show

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0501

    For Part (b1), by definition, we have

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0502
    By Lemma A.2(b), the first term is bounded by
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0503
    as required. Under Assumption 2.1(c), the second term is bounded by
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0504
    as required.

    For Part (b2), we have

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0505
    By Part (a), we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0506
    Using a similar argument to that used in the proof of Part (b1), we can bound the second term by
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0507
    Combining these, we have the required result for Part (b2). urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0508

    For urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0509, we define
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0510
    We define urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0511 to be the urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0512th element of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0513 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0514 to be the kth element of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0515, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0516. Similarly, we define urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0517 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0518.

    Lemma A.4.Under Assumptions 2.1, the following hold: (a) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0519urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0520; (b) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0521, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0522; (c) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0523, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0524; (d) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0525, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0526; (e) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0527; (f) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0528; (g) urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0529.

    Proof.Part (a). A direct calculation shows that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0530. We bound urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0531 by

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0532
    By Lemma A.3(a), we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0533
    By Lemma A.2 and Assumption 2.1, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0534
    Finally, the last term is
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0535
    as required.

    Part (b) is an immediate corollary of Part (a).

    Part (c). First, note that under Assumption 2.1 we have

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0536
    where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0537. It follows immediately that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0538
    as required. Also, the desired result follows because
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0539
    where the second equality holds by Part (a).

    Part (d). The desired result urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0540 follows from (A.12) and by direct calculation. For the second desired result, note that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0541. First, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0542 since urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0543 by urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0544 and by Part (g), which we prove later. Next, by definition,

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0545
    Because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0546, where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0547 is defined above Lemma A.1, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0548
    and
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0549
    Therefore, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0550
    as required.

    Part (e). Note that

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0551
    The required result follows because
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0552
    as required.

    Part (f) follows by Lemma A.3(b2).

    Part (g). By definition, we have

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0553
    Here, the second equality holds because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0554 where urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0555 is defined above Lemma A.1, and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0556 is defined in A.8 :
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0557
    and
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0558
    Combining the bounds of urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0559 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0560 we have the desired result for Part (g). urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0561

    Proof of (A.6).The required result follows if we show

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0562
    Note that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0563
    The first term is bounded by
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0564
    where the first equality holds by Lemma A.4(c)–(e) and the last equality holds because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0565. The second term is bounded by
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0566
    where the first equality holds by Lemma A.4(c), (d) and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0567, and the last equality holds because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0568. Combining these two, we have the required result
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0569
    The second term follows in similar fashion and we omit it. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0570

    Proof of (A.7).The required result follows, if we show

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0571
    which is established by the following three steps.
    • Step 1. We show
      urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0572
    • Step 2. By (A.6), we have
      urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0573
    • Step 3. We show
      urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0574

    Proof of Step 1.Note that because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0575 is a diagonal matrix,

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0576
    Then, the required result for Step 1 follows if we show
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0577
    The required result follows because
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0578
    where the last line holds by Lemma A.4(b)–(d) and the condition urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0579urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0580

    Proof of Step 3.We show

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0581
    The other required result urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0582 follows in similar fashion and we omit the derivation. Note that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0583
    For the first term, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0584
    where the first equality holds by Lemma A.4(c), (d) and (g) and the last equality holds by the condition urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0585. For the second term, note that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0586
    where the second equality holds by Lemma A.4(c), (d) and (f), and the last equality holds by the condition urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0587. Then, we have all of the desired results for Part (c). urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0588

    APPENDIX B:: PROOFS OF THE LIMIT DISTRIBUTION RESULTS, THEOREMS 2.2, 2.4 AND 2.6

    In this section, we provide proofs of Theorems 2.2, 2.4 and 2.6. These proofs are very similar to the proofs of the corresponding results in MPP and therefore we provide just an outline of the proofs here.

    Proof of Theorem 2.2.Because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0589, we can write

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0590
    Direct calculation shows that under the assumptions of the theorem, we have the following joint limits
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0591
    and the central limit theorem (e.g. Moon and Phillips, 1999)
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0592
    thereby giving the required result.urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0593

    Proof of Theorem 2.4.For the required result of the theorem, it is enough to show that

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0594
    Let urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0595. Then, urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0596, and we can rewrite urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0597 as
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0598
    where
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0599
    We can follow the proof in MPP (pp. 449–450) and deduce that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0600
    as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0601 with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0602, which proves the desired result. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0603

    Proof of Theorem 2.6.The required result is a consequence of Lemmata A.5 and A.6. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0604

    Lemma A.5.Let Assumption 2.1 hold. Then, as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0605 with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0606, we have

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0607

    Proof.The proof is similar to the proof of Lemma 11 of MPP and is omitted. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0608

    Lemma A.6.Let Assumption 2.1 hold. Then, as urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0609 with urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0610 the following hold:

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0611
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0612
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0613

    Proof.The proofs of Parts (b) and (c) are similar to those of Lemma 12(b) and (c) of MPP, and are omitted.

    Part (a). First, note from

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0614
    that
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0615
    Because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0616 we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0617
    Then,
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0618
    Under the assumptions of the lemma,
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0619
    and
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0620
    leading to the required result for Part (a). urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0621

    APPENDIX C:: PROOF OF THEOREM 2.7

    Proof of Theorem 2.7.We provide a sketch of the proof. Note that under Assumption 2.2, the following hold:

    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0622
    Define urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0623 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0624 Then,
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0625
    and
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0626
    Because urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0627 under Assumption 2.1, we have
    urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0628
    with probability approaching one. These imply that urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0629 satisfies the properties in Lemmata 8, 10 and 14 of MPP, while urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0630 and urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0631 satisfy the properties in Lemmata 8(a), 8(b), 10(a) and 14(a)–(d) of MPP. The desired results follow by similar arguments to those used in Theorems 8, 10 and 15 of MPP. urn:x-wiley:13684221:media:ectj12030:ectj12030-math-0632

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