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Shumway Stoffer Time_Series_Analysis_and_Its_Applications__With_R_Examples 3rd edition (1)

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362 6 State-Space Models

Table 6.2. Comparison of Standard Errors

Asymptotic Bootstrap

Parameter MLE Standard Error Standard Error

φ .865 .223 .463

α −.686 .487 .557

b .788 .226 .821

σ w .115 .107 .216

σ v 1.135 .147 .340

in the observation equation, A t = z t , Γ = α, R = σv, 2 and S = 0. The parameter

vector is Θ = (φ, α, b, σ w , σ v ) ′ . The results of the Newton–Raphson

estimation procedure are listed in Table 6.2. Also shown in the Table 6.2

are the corresponding standard errors obtained from B = 500 runs of the

bootstrap. These standard errors are simply the standard deviations of the

bootstrapped estimates, that is, the square root of ∑ B

b=1 (Θ∗ ib − ¯Θ i ∗)2 /(B−1),

where Θ i , represents the ith parameter, i = 1, . . . , 5, and ¯Θ i ∗ = ∑ B

b=1 Θ∗ ib /B.

The asymptotic standard errors listed in Table 6.2 are typically much

smaller than those obtained from the bootstrap. For most of the cases, the

bootstrapped standard errors are at least 50% larger than the corresponding

asymptotic value. Also, asymptotic theory prescribes the use of normal

theory when dealing with the parameter estimates. The bootstrap, however,

allows us to investigate the small sample distribution of the estimators and,

hence, provides more insight into the data analysis.

For example, Figure 6.9 shows the bootstrap distribution of the estimator

of φ in the upper left-hand corner. This distribution is highly skewed with

values concentrated around .8, but with a long tail to the left. Some quantiles

are −.09 (5%), .11 (10%), .34 (25%), .73 (50%), .86 (75%), .96 (90%), .98

(95%), and they can be used to obtain confidence intervals. For example, a

90% confidence interval for φ would be approximated by (−.09, .96). This

interval is ridiculously wide and includes 0 as a plausible value of φ; we will

interpret this after we discuss the results of the estimation of σ w .

Figure 6.9 shows the bootstrap distribution of ̂σ w in the lower right-hand

corner. The distribution is concentrated at two locations, one at approximately

̂σ w = .25 (which is the median of the distribution of values away from

0) and the other at ̂σ w = 0. The cases in which ̂σ w ≈ 0 correspond to deterministic

state dynamics. When σ w = 0 and |φ| < 1, then β t ≈ b for large

t, so the approximately 25% of the cases in which ̂σ w ≈ 0 suggest a fixed

state, or constant coefficient model. The cases in which ̂σ w is away from zero

would suggest a truly stochastic regression parameter. To investigate this

matter further, the off-diagonals of Figure 6.9 show the joint bootstrapped

estimates, (̂φ, ̂σ w ), for positive values of ̂φ ∗ . The joint distribution suggests

̂σ w > 0 corresponds to ̂φ ≈ 0. When φ = 0, the state dynamics are given by

β t = b + w t . If, in addition, σ w is small relative to b, the system is nearly de-

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