4.7 Article

SPITZER OBSERVATIONS OF EXOPLANETS DISCOVERED WITH THE KEPLER K2 MISSION

期刊

ASTROPHYSICAL JOURNAL
卷 822, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.3847/0004-637X/822/1/39

关键词

planets and satellites: dynamical evolution and stability; planets and satellites: gaseous planets

资金

  1. National Aeronautics and Space Administration
  2. National Science Foundation
  3. Wide-field Infrared Survey Explorer
  4. joint project of the University of California, Los Angeles
  5. Jet Propulsion Laboratory/California Institute of Technology
  6. NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute

向作者/读者索取更多资源

We have used the Spitzer Space Telescope to observe two transiting planetary systems orbiting low-mass stars discovered in the Kepler K2 mission. The system K2-3 (EPIC 201367065) hosts three planets, while K2-26 (EPIC 202083828) hosts a single planet. Observations of all four objects in these two systems confirm and refine the orbital and physical parameters of the planets. The refined orbital information and more precise planet radii possible with Spitzer will be critical for future observations of these and other K2 targets. For K2-3b we find marginally significant evidence for a transit timing variation between the K2 and Spitzer epochs.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据