2023MNRAS.524.4801K

Astronomy is presently experiencing profound growth in the deployment of machine learning to explore large data sets. However, transient quasi-periodic oscillations (QPOs) that appear in power density spectra of many X-ray binary (XRB) system observations are an intriguing phenomena heretofore not explored with machine learning. In light of this, we propose and experiment with novel methodologies for predicting the presence and properties of QPOs to make the first ever detections and characterizations of QPOs with machine learning models. We base our findings on raw energy spectra and processed features derived from energy spectra using an abundance of data from the NICER and Rossi X-ray Timing Explorer space telescope archives for two black hole low-mass XRB sources, GRS 1915+105 and MAXI J1535-571. We advance these non-traditional methods as a foundation for using machine learning to discover global inter-object generalizations between - and provide unique insights about - energy and timing phenomena to assist with the ongoing challenge of unambiguously understanding the nature and origin of QPOs. Additionally, we have developed a publicly available PYTHON machine learning library, QPOML, to enable further machine learning aided investigations into QPOs.