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      A Machine Learning Approach For Classifying Low-mass X-ray Binaries Based On Their Compact Object Nature

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          Abstract

          Low Mass X-ray binaries (LMXBs) are binary systems where one of the components is either a black hole or a neutron star and the other is a less massive star. It is challenging to unambiguously determine whether a LMXB hosts a black hole or a neutron star. In the last few decades, multiple observational works have tried, with different levels of success, to address this problem. In this paper, we explore the use of machine learning to tackle this observational challenge. We train a random forest classifier to identify the type of compact object using the energy spectrum in the energy range 5-25 keV obtained from the Rossi X-ray Timing Explorer archive. We report an average accuracy of 87+/-13 in classifying the spectra of LMXB sources. We further use the trained model for predicting the classes for LMXB systems with unknown or ambiguous classification. With the ever-increasing volume of astronomical data in the X-ray domain from present and upcoming missions (e.g., SWIFT, XMM-Newton, XARM, ATHENA, NICER), such methods can be extremely useful for faster and robust classification of X-ray sources and can also be deployed as part of the data reduction pipeline.

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          Author and article information

          Journal
          12 December 2020
          Article
          2012.06934
          e455d568-367e-420a-aaf2-f0703e840e7e

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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          Custom metadata
          16 pages, 10 figures, 7 tables, Accepted for publication in MNRAS main journal
          astro-ph.HE

          High energy astrophysical phenomena
          High energy astrophysical phenomena

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