ExplorerSpace ScienceAstrophysics
Research PaperResearchia:202607.07049

CausticFlow: An Efficient Machine Learning Framework Combining Neural Differential Equations and Normalizing Flows for Binary Microlensing Parameter Inference

Haibin Ren

Abstract

We introduce CausticFlow, a machine learning framework that combines neural controlled differential equations with normalizing flows to infer binary microlensing parameters. This architecture naturally handles irregularly sampled time series and data gaps while flexibly capturing strongly correlated and multimodal posterior distributions. Trained on simulated KMTNet-like light curves, CausticFlow generates posterior samples in a fraction of a second, with maximum-a-posteriori estimates achieving...

Submitted: July 7, 2026Subjects: Astrophysics; Space Science

Description / Details

We introduce CausticFlow, a machine learning framework that combines neural controlled differential equations with normalizing flows to infer binary microlensing parameters. This architecture naturally handles irregularly sampled time series and data gaps while flexibly capturing strongly correlated and multimodal posterior distributions. Trained on simulated KMTNet-like light curves, CausticFlow generates posterior samples in a fraction of a second, with maximum-a-posteriori estimates achieving typical precisions of 17%\sim17\% for the mass ratio qq and 3%\sim3\% for the projected separation ss. When used as a proposal distribution for downstream local optimization, the framework improves these precisions to <5%<5\% and <1%<1\%, respectively, and recovers model χ2χ^2 for 80%\sim80\% of simulated events. We test the generalizability of the framework on 10 real binary lensing events characterized by higher-order effects, varied cadences, and real-world noise. Despite these mismatches between simulation and reality, CausticFlow successfully recovers the model parameters, light-curve morphology, and lensing geometry for 7 of the 10 events after simple local refinement, achieving precision levels comparable to those found for simulated data in 10 CPU minutes per event. These results demonstrate that CausticFlow acts as a fast and robust proposal engine, bridging the gap between the rapid influx of data and the need for systematic modeling in large-scale microlensing surveys such as Roman, CSST, and ET.


Source: arXiv:2607.04955v1 - http://arxiv.org/abs/2607.04955v1 PDF: https://arxiv.org/pdf/2607.04955v1 Original Link: http://arxiv.org/abs/2607.04955v1

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Date:
Jul 7, 2026
Topic:
Space Science
Area:
Astrophysics
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