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FALCO: Foundation Model of Astronomical Light Curves for Time Domain Astronomy. Implementation and Applications on Kepler Data

  • Authors: Xiaoxiong Zuo, Yihan Tao, Yang Huang, Zhixuan Kang, Huaxi Chen, Chenzhou Cui, Jiashu Pan, Xiao Kong, Yuan-Sen Ting, Xiaoyu Tang, Henggeng Han, Haiyang Mu, Yunfei Xu, Dongwei Fan, Guirong Xue, Ali Luo, Jifeng Liu

Xiaoxiong Zuo et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 1.

Light curves of different classes derived from FITS files obtained via MAST from a single quarter of Kepler observations. Panels are labeled as (a) APERIODIC, (b) CONTACT ROT, (c) DSCT BCEP, (d) ECLIPSE, (e) SOLARLIKE, (f) GDOR SPB, (g) RRLYR CEPHEID, and (h) NONVARIABLE. Visible gaps in some light curves are due to observational or instrumental effects.

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