Gravitational lensing is the relativistic effect generated by massive bodies, which bend the space-time surrounding them. It is a deeply investigated topic in astrophysics and allows validating theoretical relativistic results and studying faint astrophysical objects that would not be visible otherwise. In recent years Machine Learning methods have been applied to support the analysis of the gravitational lensing phenomena by detecting lensing effects in data sets consisting of images associated with brightness variation time series. However, the state-of-art approaches either consider only images and neglect time-series data or achieve relatively low accuracy on the most difficult data sets. This paper introduces DeepGraviLens, a novel multi-modal network that classifies spatio-temporal data belonging to one non-lensed system type and three lensed system types. It surpasses the current state of the art accuracy results by $\approx$ 19% to $\approx$ 43%, depending on the considered data set. Such an improvement will enable the acceleration of the analysis of lensed objects in upcoming astrophysical surveys, which will exploit the petabytes of data collected, e.g., from the Vera C. Rubin Observatory.
翻译:引力透镜是巨型物体产生的相对效应,使空间时间围绕它们。这是一个在天体物理学中进行深入调查的专题,可以验证理论相对论结果,并研究否则看不到的微弱天体物理物体。近年来,机器学习方法被用于支持引力透镜现象的分析,通过检测由光度变化时间序列相关图像组成的数据集中的透镜效应。然而,最先进的方法要么只考虑图像,忽略时间序列数据,要么在最困难的数据集上实现相对低的精确度。本文介绍DeepGraviLens,这是一个全新的多模式网络,将属于一个非孤单系统类型和三个透视系统类型的数据分类为spatio-时空数据。它比目前艺术精确率高,用$\approx 19%至 $approx 43%,这取决于所考虑的数据集。这种改进将加快对即将进入天体物理测量的透镜对象的分析,该观测将利用Petrobya.a.