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Nonparametric Conditional Density Estimation in a High-Dimensional egression Setting

机译:高维出口设置中的非参数条件密度估计

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摘要

In some applications (e.g., in cosmology and economics), the regression E[Z vertical bar x] is not adequate to represent the association between a predictor x and a response Z because of multi-modality and asymmetry of f (Z vertical bar x); using the full density instead of a single point estimate can then lead to less bias in subsequent analysis. As of now, there are no effective ways of estimating f (Z vertical bar x) when x represents high-dimensional, complex data. In this article, we propose a new nonparametric estimator of f (Z vertical bar x) that adapts to sparse (low-dimensional) structure in x. By directly expanding f (Z vertical bar x) in the eigenfunctions of a kernel-based operator, we avoid tensor products in high dimensions as well as ratios of estimated densities. Our basis functions are orthogonal with respect to the underlying data distribution, allowing fast implementation and tuning of parameters. We derive rates of convergence and show that the method adapts to the intrinsic dimension of the data. We also demonstrate the effectiveness of the series method on images, spectra, and an application to photometric redshift estimation of galaxies. Supplementary materials for this article are available online.
机译:在一些应用(例如,在宇宙学和经济学中),回归E [z垂直条x]不足以表示预测器x和响应z之间的关联,因为f的多模态和f(z垂直条x );然后,使用完整的密度而不是单点估计可以导致随后的分析中的偏差更少。截至目前,当X表示高维,复杂数据时,没有有效的方法估计F(Z垂直条X)。在本文中,我们提出了一种新的F(Z垂直条X)的非参数估计器,其适应X中的稀疏(低维)结构。通过在基于内核的操作员的特征函数中直接扩展F(Z垂直条X),我们避免了高尺寸的张量产品以及估计密度的比率。我们的基本函数与底层数据分布正交,允许快速实现和调整参数。我们得出收敛率,并表明该方法适应数据的内在维度。我们还展示了串联方法对图像,光谱射频估计的串联方法的有效性。本文的补充材料可在线获得。

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