Searching for Quasi-Periodic Eruptions using machine learning

R. Webbe, A. Young
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Abstract

Quasi-Periodic Eruptions (QPEs) are a rare phenomenon in which the X-ray emission from the nuclei of galaxies shows a series of large amplitude flares. Only a handful of QPEs have been observed but the possibility remains that there are as yet undetected sources in archival data. Given the volume of data available a manual search is not feasible, and so we consider an application of machine learning to archival data to determine whether a set of time-domain features can be used to identify further lightcurves containing eruptions. Using a neural network and 14 variability measures we are able to classify lightcurves with accuracies of greater than $94{{\%}}$ with simulated data and greater than $98{{\%}}$ with observational data on a sample consisting of 12 lightcurves with QPEs and 52 lightcurves without QPEs. An analysis of 83,531 X-ray detections from the XMM Serendipitous Source Catalogue allowed us to recover lightcurves of known QPE sources and examples of several categories of variable stellar objects.
用机器学习搜索准周期性喷发
准周期爆发(qpe)是一种罕见的现象,在这种现象中,星系核的x射线发射显示出一系列大振幅的耀斑。只有少数qpe被观察到,但仍然有可能在档案数据中存在尚未发现的来源。考虑到可用的数据量,手动搜索是不可行的,因此我们考虑将机器学习应用于档案数据,以确定是否可以使用一组时域特征来识别包含火山爆发的进一步光曲线。使用神经网络和14个可变性度量,我们能够在由12条带qpe的光曲线和52条不带qpe的光曲线组成的样本上,对模拟数据的光曲线分类精度大于$94{{\%}}$,对观测数据的光曲线分类精度大于$98{{\%}}$。通过对来自XMM偶然源目录的83,531次x射线探测的分析,我们恢复了已知QPE源的光曲线和几类变星物体的例子。
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