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关注这篇论文的作者
Arya Farahi
Conghao Zhou
Ritwik Vashistha

OASIS:基于分布匹配的观测感知仿真推断

研究问题
当观测数据经过测量误差、选择效应等观测流程变换,而仿真器只生成潜在无噪声量时,如何直接对观测数据分布进行仿真推断。
方法与思路
作者提出将观测模型显式嵌入仿真器,用最大均值差异(MMD)损失对先验样本重加权构造伪后验,比较观测数据与正向仿真观测的经验分布,避免手工摘要与神经代理。
材料陈述的贡献
摘要称给出蒙特卡洛一致性、经验伪后验收敛到总体对应物、后验在MMD可识别参数集上集中的理论保证,并在变量误差回归与多波段星系团宇宙学应用中展示稳健参数恢复与校准不确定性。
阅读关注点
应核对观测模型嵌入的具体形式、MMD核与权重构造、可识别性条件、理论保证的假设,以及宇宙学应用中缩放关系、异方差误差与选择函数的设定。
阅读边界
这是arXiv预印本,未经同行评审或期刊接收;摘要未说明仿真器细节、样本规模、计算成本及与替代方法的系统比较,不能据此判断方法优越性。

原文摘要

We introduce OASIS, a simulation-based inference framework for scientific settings where observations are distorted by measurement error, selection effects, and other survey-specific transformations. In many real applications, simulators generate latent, noiseless quantities, while the data are observed only after passing through a complex observational pipeline. Standard simulation-based inference methods often ignore this distinction, comparing observations to idealized simulator outputs or relying on low-dimensional summaries that can miss important structure. OASIS addresses this mismatch by explicitly embedding the observation model into the simulator and performing inference directly at the level of observed-data distributions. The method constructs a pseudo-posterior by reweighting prior samples according to a maximum mean discrepancy (MMD) loss between the empirical distributions of the observed data and forward-simulated observations, thereby avoiding both handcrafted summaries and learned neural surrogates. We provide theoretical guarantees for Monte Carlo consistency, convergence of the empirical pseudo-posterior to its population counterpart, and posterior concentration on the MMD-identified parameter set, with consistency for the true parameter under correct specification and identifiability. In controlled errors-in-variables regression experiments, OASIS delivers robust parameter recovery and well-calibrated uncertainty under heterogeneous and non-Gaussian measurement noise. We then demonstrate the method on a realistic cosmological application involving galaxy cluster observations across multiple wavelengths, in which latent physical properties are linked to observables through nonlinear scaling relations, heteroscedastic errors, selection functions, and incomplete coverage.

笔记与分组
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