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本页整理公开书目信息,不生成学术质量评分。AI 解读根据题名及所注明的摘要或原文片段生成,未完成全文核验,可能有误;具体假设、证明与结论请核对原文。摘要保留来源文本,未经模型改写。

DOI 首次登记不等于接收或发表日期。部分更正、评论等条目没有独立摘要;缺少可靠材料时保留待补状态。

引用量采用 OpenAlex 单条关联记录,不合计多个记录;关联记录可能包含正式发表版本,不等于此版本单独引用。缺失不视为零,引用指标不代表论文质量。

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分类依据与纠错

AI 根据所提供的论文材料归类:摘要研究一般泊松强度估计,应用是高能天体物理,缺乏所列领域的直接依据。

反馈分类问题

正在核对关联版本…

代码、数据与补充材料

正在核对对应版本的资源…

关注这篇论文的作者
Eric D. Kolaczyk

泊松过程的贝叶斯多尺度模型

研究问题
如何估计一维非齐次泊松过程的离散化强度函数,同时利用不同尺度的信息,并以可计算方式刻画强度的多尺度结构?
方法与思路
作者通过递归二分划分构造树状似然模型,在节点设置混合先验,再混合不同树,并用经验贝叶斯方法选择混合参数。
材料陈述的贡献
摘要称,平方误差损失下可得到贝叶斯最优估计的闭式递归表达;树混合还用于诱导先验平稳性与改善数据分辨率下的逼近。
阅读关注点
应核对树混合与节点先验的定义、递归计算的成本、经验贝叶斯参数选择,以及先验平稳性与过程非齐次性的区别。
阅读边界
仅据 OpenAlex 索引摘要,稿件版本未注明,不能推断刊本变化;模拟与天体物理应用未给出数值,亦不能直接外推到金融高频数据。

原文摘要

I introduce a class of Bayesian multiscale models (BMSM's) for one-dimensional inhomogeneous Poisson processes. The focus is on estimating the (discretized) intensity function underlying the process. Unlike the usual transform-based approach at the heart of most wavelet-based methods for Gaussian data, these BMSM's are constructed using recursive dyadic partitions (RDP's) within an entirely likelihood-based framework. Each RDP may be associated with a binary tree, and a new multiscale prior distribution is introduced for the unknown intensity through the placement of mixture distributions at each of the nodes of the tree. The concept of model mixing is then applied to a complete collection of such trees. In addition to allowing for the inclusion of full location/scale information in the model, this last step also is fundamental both in inducing stationarity in the prior distribution and in enabling a given intensity function to be approximated at the resolution of the data. Under squared-error loss, a closed-form recursive expression for the Bayes optimal estimator is derived, which makes computationally efficient implementation possible. The mixing parameters in the prior distribution can be interpreted as the “fraction of homogeneity” in the underlying intensity function at each scale, and I provide an empirical Bayes approach to eliciting their values, resulting in the ability to quantify multiscale structure in the data. The practical performance of the overall procedure is investigated through a series of simulations and illustrated using a real-data example from the field of high-energy astrophysics.

笔记与分组