The results of surface gravity parameters (log g) derived from the analysis of the full Kepler dataset using the FALCO model.
Xiaoxiong Zuo ; Yihan Tao
After self supervised pre training, the FALCO model is used for analyzing scientific tasks. This dataset is the log g parameter obtained from the analysis of stellar surface gravity parameters using the FALCO model on all Kepler light curve data. This CSV dataset contains Kepler ID, namely kic, as well as log g values.
Files
kepler_logg.csv
3.62 MB
Paper Information
Paper Title:
FALCO: Foundation model of Astronomical Light Curves for time dOmain astronomy. Implementation and Applications on Kepler data
Publication:
AJ
Identifiers
CSTR:
11379.11.101577
DOI:
10.12149/101577
VO Identifier:
ivo://China-VO/paperdata/101577
Publication Date:
2025-10-14
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Citations
Xiaoxiong Zuo et al. 2025. The results of surface gravity parameters (log g) derived from the analysis of the full Kepler dataset using the FALCO model.. Version 1.0. https://doi.org/10.12149/101577
@misc{10.12149/101577,
doi = {10.12149/101577},
url = {https://doi.org/10.12149/101577},
author = {Xiaoxiong Zuo},
title = {The results of surface gravity parameters (log g) derived from the analysis of the full Kepler dataset using the FALCO model.},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2025}
}
doi = {10.12149/101577},
url = {https://doi.org/10.12149/101577},
author = {Xiaoxiong Zuo},
title = {The results of surface gravity parameters (log g) derived from the analysis of the full Kepler dataset using the FALCO model.},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2025}
}
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Main
This DOI represents all versions, and will always resolve to the latest one.
2025-10-14