7–11 Jul 2025
Teaching and Learning Centre (TLC)
Europe/London timezone

Uncovering Hidden Extragalactic Flares and Dips from the Chandra Archive with Machine Learning

9 Jul 2025, 09:20
12m
Teaching and Learning Centre (TLC)

Teaching and Learning Centre (TLC)

Durham University South Road Durham DH1 3LS
Talk Chandra and XMM-Newton at 25 - Utilising Several Decades of X-ray observation Chandra and XMM-Newton at 25 - Utilising Several Decades of X-ray observation

Description

We present a novel representation learning method for downstream tasks like anomaly detection or unsupervised classification in high-energy datasets. This enabled the discovery of a new extragalactic fast X-ray transient (FXT) in Chandra archival data, XRT 200515, a needle-in-the-haystack event and the first Chandra FXT of its kind. Recent serendipitous discoveries in X-ray astronomy, including FXTs from binary neutron star mergers and an extragalactic planetary transit candidate, highlight the need for systematic transient searches in X-ray archives. We introduce new event file representations, $E-t$ Maps and $E-t-dt$ Cubes, that effectively encode both temporal and spectral information, enabling the seamless application of machine learning to variable-length event file time series. Our unsupervised learning approach employs PCA or sparse autoencoders to extract low-dimensional, informative features from these data representations, followed by clustering in the embedding space with DBSCAN. New transients are identified within transient-dominant clusters or through nearest-neighbor searches around known transients, producing a catalog of 3559 candidates (3447 flares and 112 dips). XRT 200515 exhibits unique temporal and spectral variability, including an intense, hard $<$10s initial burst, followed by spectral softening in an $\sim$800s oscillating tail. We interpret XRT 200515 as either an unusual magnetar flare observed at low X-ray energies or the first extragalactic Type I X-ray burst from a faint, previously unknown LMXB in the LMC. Our method extends to datasets from other observatories such as XMM-Newton, Swift-XRT, eROSITA, Einstein Probe, and upcoming missions like AXIS.

Primary author

Steven Dillmann (Stanford University)

Co-authors

Dr Rafael Martinez-Galarza (Center for Astrophysics | Harvard & Smithsonian) Dr Roberto Soria (INAF) Dr Rosanne Di Stefano (Center for Astrophysics | Harvard & Smithsonian) Dr Vinay Kashyap (Center for Astrophysics | Harvard & Smithsonian)

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