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arXiv 2109.03466math.STstat.TH

多元异方差经验贝叶斯方法:基于非参数最大似然估计

Multivariate, Heteroscedastic Empirical Bayes via Nonparametric Maximum Likelihood

Jake A. Soloff, Adityanand Guntuboyina, Bodhisattva Sen

AI总结:

本研究将非参数最大似然估计扩展到多元异方差误差,提出一种经验贝叶斯去噪方法,具有近最优性能,并应用于天文学和层次线性模型,展示了其自适应性和优势。

摘要:

多元、异方差的误差在许多大规模去噪问题中使统计推断变得复杂。经验贝叶斯方法在此类情境中具有吸引力,但标准的参数化方法依赖于对先验分布形式的假设,这些假设难以证明其合理性,并且引入了不必要的调参参数。我们将用于高斯位置混合密度的非参数最大似然估计(NPMLE)扩展到允许多元、异方差的误差。NPMLE通过求解一个无限维凸优化问题来估计任意先验;我们证明该凸优化问题可以近似为一个有限维版本,从而易于求解。基于NPMLE的经验贝叶斯后验均值具有低遗憾,意味着它们紧密地逼近在已知真实先验情况下计算出的Oracle后验均值。我们证明了一个Oracle不等式,表明该经验贝叶斯估计器在无先验知识去噪中的性能接近最优水平(仅差对数因子)。我们提供了NPMLE估计观测边际密度的平均Hellinger精度的有限样本界。我们还展示了NPMLE在解卷积中的自适应性和近最优性。我们将我们的方法应用于天文学中的两个去噪问题:构建了银河系中140万颗恒星的全数据驱动的颜色-星等图,并研究了红团簇中27,000颗恒星的19个化学丰度比的分布。我们还将我们的方法应用于层次线性模型,展示了在教育数据集和微阵列数据集上回归系数的非参数收缩的优势。

英文摘要:

Multivariate, heteroscedastic errors complicate statistical inference in many large-scale denoising problems. Empirical Bayes is attractive in such settings, but standard parametric approaches rest on assumptions about the form of the prior distribution which can be hard to justify and which introduce unnecessary tuning parameters. We extend the nonparametric maximum likelihood estimator (NPMLE) for Gaussian location mixture densities to allow for multivariate, heteroscedastic errors. NPMLEs estimate an arbitrary prior by solving an infinite-dimensional, convex optimization problem; we show that this convex optimization problem can be tractably approximated by a finite-dimensional version. The empirical Bayes posterior means based on an NPMLE have low regret, meaning they closely target the oracle posterior means one would compute with the true prior in hand. We prove an oracle inequality implying that the empirical Bayes estimator performs at nearly the optimal level (up to logarithmic factors) for denoising without prior knowledge. We provide finite-sample bounds on the average Hellinger accuracy of an NPMLE for estimating the marginal densities of the observations. We also demonstrate the adaptive and nearly-optimal properties of NPMLEs for deconvolution. We apply our method to two denoising problems in astronomy, constructing a fully data-driven color-magnitude diagram of 1.4 million stars in the Milky Way and investigating the distribution of 19 chemical abundance ratios for 27 thousand stars in the red clump. We also apply our method to hierarchical linear models, illustrating the advantages of nonparametric shrinkage of regression coefficients on an education data set and on a microarray data set.

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