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A Bias-reduced log-periodogram regression estimator for the long-memory parameter

机译:长记忆参数的偏倚减少对数周期回归估计

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In this paper, we propose a simple bias-reduced log-periodogram regression estimator, (d-tilde)_r, or the long-memory parameter, d, that eliminates the first- and higher-order biases of the Geweke and Porter-Hudak (1983)(GPH) estimator. The bias-reduced estimator is the same as the GPH estimator except that one includes frequencies to the power 2k for k = 1, …, r, for some positive integer r, as additional regressors in the pseudo-regression model that yields the GPH estimator. The reduction in bias is obtained using assumptions on the spectrum only in a neighborhood of the zero frequency. Following the work of Robinson (1995b) and Hurvich, Deo, and Brodsky (1998) we establish the asymptotic bias, variance, and mean-squared error (MSE) of (d-tilde)_r determine the asymptotic MSE optimal choice of the number of frequencies, m, to include in the regression, and establish the asymptotic normality of (d-tilde)_r, There results show that the bias of (d-tilde)_r goes to zero at a faster rate than that of the GPH estimator when the normalized spectrum at zero is sufficiently smooth, but that its variance only is increased by a multiplicative constant. We show that the bias-reduced estimator (d-tilde)_r attains the optimal rate of convergence for a class of spectral densities that includes those that are smooth of order s ≥ 1 at zero when r ≥ (s - 2)/2 and m is chosen appropriately. For s > 2, the GPH estimator does not attain this rate. The proof uses results of Giraitis, Robinson, and Samarov (1997). We specify a data-dependent plug-in method for selecting the number of frequencies m to minimize asymptotic MSE for a given value of r. Some Monte Carlo simulation results for stationary Gaussian ARFIMA (1, d, 1) and (2, d, 0) models show that the bias-reduced estimators perform well relative to the standard log-periodogram regression estimator.
机译:在本文中,我们提出了一种简单的减少偏倚的对数周期图回归估计量(d-tilde)_r或长记忆参数d,它消除了Geweke和Porter-Hudak的一阶和高阶偏置。 (1983)(GPH)估算器。减少偏倚的估算器与GPH估算器相同,不同之处在于,对于某些正整数r,对于k = 1,...,r包含幂2k的频率,作为产生GPH估算器的伪回归模型中的其他回归器。仅在零频率附近使用频谱上的假设才能获得偏置的降低。继Robinson(1995b)和Hurvich,Deo和Brodsky(1998)的工作之后,我们确定(d-tilde)_r的渐近偏差,方差和均方误差(MSE)确定了渐近MSE数的最佳选择的频率m包含在回归中并建立(d-tilde)_r的渐近正态性,结果表明(d-tilde)_r的偏差以比GPH估计器更快的速率变为零当归一化频谱在零处足够平滑时,但其方差仅增加一个乘法常数。我们表明,对于一类光谱密度(包括当r≥(s-2)/ 2且在零时光滑s≥1的那些光谱密度),降低偏倚的估计量(d-tilde)_r可获得最佳收敛速度。 m适当选择。对于s> 2,GPH估算器无法达到该速率。该证据使用了Giraitis,Robinson和Samarov(1997)的结果。我们指定了一种依赖数据的插件方法,用于选择频率数量m,以在给定r值时将渐近MSE最小化。平稳高斯ARFIMA(1,d,1)和(2,d,0)模型的一些蒙特卡罗模拟结果表明,相对于标准对数周期回归回归估计器,减少偏倚的估计器性能良好。

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