TESS-miner 100-pc M-dwarf Sample
收藏Zenodo2025-06-25 更新2026-05-26 收录
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https://zenodo.org/doi/10.5281/zenodo.15733570
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This dataset was used in the analysis presented in Glusman et al. (2025), which investigates the occurrence rates of giant planets orbiting low-mass stars observed by TESS. It contains astrometric, photometric, and stellar parameter data for 149,316 M dwarfs, compiled from Gaia DR3 and the TESS Input Catalog (TIC), as well as derived quantities such as absolute magnitudes, color indices, and stellar properties computed using the empirical relations of Mann et al. (2015, 2019). Each star is also labeled with its spectral type and a classification output from the TESS-Miner pipeline. The dataset provides the foundation for the sample definition and occurrence rate modeling described in the publication.
本数据集被应用于Glusman等人(2025)的分析研究中,该研究针对凌日系外行星巡天卫星(Transiting Exoplanet Survey Satellite, TESS)观测的低质量恒星周围巨行星的出现率展开探讨。数据集包含149316颗M型矮星的天体测量、测光以及恒星参数数据,这些数据汇编自盖亚第三批数据发布(Gaia Data Release 3, Gaia DR3)与TESS输入星表(TESS Input Catalog, TIC);同时还包含通过Mann等人(2015、2019)的经验关系式计算得到的衍生量,如绝对星等、色指数以及恒星物理属性。每颗恒星均标注了其光谱型,以及来自TESS-Miner流水线的分类结果。本数据集为该论文中所述的样本定义与行星出现率建模工作提供了核心基础。
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Zenodo创建时间:
2025-06-25



