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TTC: Transformer-based TDE Classifier for the Wide Field Survey Telescope (WFST)

Ranfang Zheng, Zheyu Lin, Xu Kong, Dezheng Meng, Zelin Xu, Lulu Fan, Ji-an Jiang, Ning Jiang, Jie Lin, Tinggui Wang, Qingfeng Zhu, Feng Li, Ming Liang, Hao Liu, Zheng Lou, Wentao Luo, Jinlong Tang, Hairen Wang, Jian Wang, Yongquan Xue, Dazhi Yao, Hong-fei Zhang, Wen Zhao, Xianzhong Zheng, Yingxi Zuo

TL;DR

We address automatic photometric identification of tidal disruption events (TDEs) from light curves alone, suitable for WFST alert streams and archives. We introduce TTC, a two-module system with a light-curve parametric fitting component and a Mgformer Transformer classifier, trained on a ZTF dataset of 7413 transients and capable of identifying TDEs within $30$ days of first detection. The Mgformer module achieves recall $0.79$ and precision $0.76$, while the parametric module achieves recall $0.72$ and precision $0.40$, enabling a tunable performance-time trade-off. In real-time ZTF tests TTC identified all spectroscopically confirmed TDEs and found roughly $20$ TDE candidates in WFST deep-field data, illustrating scalable, catalog-light TDE discovery.

Abstract

We propose the Transformer-based Tidal disruption events (TDE) Classifier (\texttt{TTC}), specifically designed to operate effectively with both real-time alert streams and archival data of the Wide Field Survey Telescope (WFST). It aims to minimize the reliance on external catalogs and find TDE candidates from pure light curves, which is more suitable for finding TDEs in faint and distant galaxies. \texttt{TTC} consists of two key modules that can work independently: (1) A light curve parametric fitting module and (2) a Transformer (\texttt{Mgformer})-based classification network. The training of the latter module and evaluation for each module utilize a light curve dataset of 7413 spectroscopically classified transients from the Zwicky Transient Facility (ZTF). The \texttt{Mgformer}-based module is superior in performance and flexibility. Its representative recall and precision values are 0.79 and 0.76, respectively, and can be modified by adjusting the threshold. It can also efficiently find TDE candidates within 30 days from the first detection. For comparison, the parametric fitting module yields values of 0.72 and 0.40, respectively, while it is $>$10 times faster in average speed. Hence, the setup of modules allows a trade-off between performance and time, as well as precision and recall. \texttt{TTC} has successfully picked out all spectroscopically identified TDEs among ZTF transients in a real-time classification test, and selected $\sim$20 TDE candidates in the deep field survey data of WFST. The discovery rate will greatly increase once the differential database for the wide field survey is ready.

TTC: Transformer-based TDE Classifier for the Wide Field Survey Telescope (WFST)

TL;DR

We address automatic photometric identification of tidal disruption events (TDEs) from light curves alone, suitable for WFST alert streams and archives. We introduce TTC, a two-module system with a light-curve parametric fitting component and a Mgformer Transformer classifier, trained on a ZTF dataset of 7413 transients and capable of identifying TDEs within days of first detection. The Mgformer module achieves recall and precision , while the parametric module achieves recall and precision , enabling a tunable performance-time trade-off. In real-time ZTF tests TTC identified all spectroscopically confirmed TDEs and found roughly TDE candidates in WFST deep-field data, illustrating scalable, catalog-light TDE discovery.

Abstract

We propose the Transformer-based Tidal disruption events (TDE) Classifier (\texttt{TTC}), specifically designed to operate effectively with both real-time alert streams and archival data of the Wide Field Survey Telescope (WFST). It aims to minimize the reliance on external catalogs and find TDE candidates from pure light curves, which is more suitable for finding TDEs in faint and distant galaxies. \texttt{TTC} consists of two key modules that can work independently: (1) A light curve parametric fitting module and (2) a Transformer (\texttt{Mgformer})-based classification network. The training of the latter module and evaluation for each module utilize a light curve dataset of 7413 spectroscopically classified transients from the Zwicky Transient Facility (ZTF). The \texttt{Mgformer}-based module is superior in performance and flexibility. Its representative recall and precision values are 0.79 and 0.76, respectively, and can be modified by adjusting the threshold. It can also efficiently find TDE candidates within 30 days from the first detection. For comparison, the parametric fitting module yields values of 0.72 and 0.40, respectively, while it is 10 times faster in average speed. Hence, the setup of modules allows a trade-off between performance and time, as well as precision and recall. \texttt{TTC} has successfully picked out all spectroscopically identified TDEs among ZTF transients in a real-time classification test, and selected 20 TDE candidates in the deep field survey data of WFST. The discovery rate will greatly increase once the differential database for the wide field survey is ready.
Paper Structure (2 sections)

This paper contains 2 sections.