Microlensify: a Transformer Based Machine Learning Classifier for Microlensing Events Trained on TESS Light Curves
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Astrophysics > Instrumentation and Methods for Astrophysics
Title:Microlensify: a Transformer Based Machine Learning Classifier for Microlensing Events Trained on TESS Light Curves
Abstract:Microlensing can reveal populations of faint compact objects that are otherwise difficult to detect. Depending on their design, all-sky surveys have the potential to search for these objects across the sky. The Transiting Exoplanet Survey Satellite (TESS), primarily designed to detect transiting exoplanets, also provides near all-sky coverage with high cadence. In this work, we use TESS data to search for microlensing candidates using both traditional and machine-learning methods and to identify associated false positives in high-cadence surveys.
Microlensify is a physics-informed, transformer-based variational autoencoder trained on simulated single-lens microlensing light curves and real TESS Sector 12 data. The model classifies events, reconstructs light curves, and estimates microlensing event durations. Applied to $\sim 5.6$ million TESS light curves, it identified between $0.036\%$ and $1.89\%$ as microlensing candidates across different TESS pipelines. After applying microlensing detection metrics and cross-matching with SIMBAD, we obtained a final list of candidates and identified false positives including long-period variables, Mira variables, cataclysmic variables, red giants, and transients. We also found Gaussian-like peaks caused by asteroid crossings, a potential source of false positives in high-cadence microlensing surveys.
The model also predicts event duration with an accuracy of $R^2 = 0.97$.
The model was further tested on published events from different ground-based microlensing surveys, confirming 92.7% as microlensing, demonstrating its applicability across surveys with different cadences.
| Subjects: | Instrumentation and Methods for Astrophysics (astro-ph.IM); Earth and Planetary Astrophysics (astro-ph.EP); Astrophysics of Galaxies (astro-ph.GA); Solar and Stellar Astrophysics (astro-ph.SR); Machine Learning (cs.LG) |
| Cite as: | arXiv:2608.19419 [astro-ph.IM] |
| (or arXiv:2608.19419v1 [astro-ph.IM] for this version) | |
| https://doi.org/10.48550/arXiv.2608.19419
arXiv-issued DOI via DataCite
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Submission history
From: Atousa Kalantari [view email][v1] Wed, 19 Aug 2026 20:11:01 UTC (4,248 KB)
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