0. For estimating the autocorrelation-range and the variance of'/> Asymptotic near-efficiency of the 'Gibbs-energy (GE) and empirical-variance'' estimating functions for fitting Matern models - II: Accounting for measurement errors via 'conditional GE mean''
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Asymptotic near-efficiency of the 'Gibbs-energy (GE) and empirical-variance'' estimating functions for fitting Matern models - II: Accounting for measurement errors via 'conditional GE mean''

机译:“Gibbs-Energy(Ge)和实验 - 方差”估算函数的渐近近效率 - II - II:通过“条件Ge意思”的测量误差核算

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摘要

Consider one realization of a continuous-time Gaussian process Z which belongs to the Matern family with known "regularity'' index nu > 0. For estimating the autocorrelation-range and the variance of Z from n observations on a fine grid, we studied in Girard (2016) the GE-EV method which simply retains the empirical variance (EV) and equates it to a candidate "Gibbs energy (GE)", i.e. the quadratic form z(T) R(-1)z/n where z is the vector of observations and R is the autocorrelation matrix for z associated with a candidate range. The present study considers the case where the observation is z plus a Gaussian white noise whose variance is known. We propose to simply bias-correct EV and to replace GE by its conditional mean given the observation. We show that the ratio of the large-n mean squared error of the resulting CGEM-EV estimate of the range-parameter to the one of its maximum likelihood estimate, and the analog ratio for the variance-parameter, have the same behavior than in the no-noise case: they both converge, when the grid-step tends to 0, toward a constant, only function of., surprisingly close to 1 provided. is not too large. We also obtain, for all., convergence to 1 of the analog ratio for the microergodic-parameter. Furthermore, we discuss possible non-normality of the noise, and the impact of a "not small enough'' grid-step. (C) 2020 Elsevier B.V. All rights reserved.
机译:考虑一种实现与已知的“规律性”指标NU> 0的母乳系列的连续高斯工艺Z的一个实现。用于估计自相关范围和来自N观察的Z的变化,我们研究过Girard(2016)简单地保留了经验方差(EV)的GE-EV方法,并将其等于候选“GIBBS能量(GE)”,即二次形式Z(T)R(-1)z / n其中z是观察矢量,R是与候选范围相关联的z的自相关矩阵。本研究考虑了观察是z加上其差所知的高斯白噪声。我们建议简单地偏见 - 正确的EV和偏见鉴于观察,通过其条件平均替换Ge。我们展示了所得CGEM-EV估计的大n平均平方误差与其最大似然估计的一个和模拟比率的比例方差参数,具有比在的相同行为无噪声案例:它们都会收敛,当网格步骤趋于0,朝向常数,唯一的功能。,惊人的靠近1。不是太大了。我们还获得了所有。,为微晶素参数的模拟比率收敛到1。此外,我们讨论可能的噪音的非正常性,以及“不够小”网格步骤的影响。(c)2020 Elsevier B.v.保留所有权利。

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