4.6 Article

The SOPHIE search for northern extrasolar planets III. A Jupiter-mass companion around HD 109246

期刊

ASTRONOMY & ASTROPHYSICS
卷 523, 期 -, 页码 -

出版社

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201014909

关键词

planetary systems; techniques: radial velocities; stars: individual: HD 109246; stars: activity; stars: abundances

资金

  1. Swiss National Science Foundation [PA00P2_126150/1]
  2. European Research Council/European Community
  3. FCT/MCTES (Portugal)
  4. POPH/FSE (EC)
  5. CNES
  6. [PTDC/CTE-AST/098528/2008]
  7. [PTDC/CTE-AST/098604/2008]
  8. Swiss National Science Foundation (SNF) [PA00P2_126150] Funding Source: Swiss National Science Foundation (SNF)

向作者/读者索取更多资源

We report the detection of a Jupiter-mass planet discovered with the SOPHIE spectrograph mounted on the 1.93-m telescope at the Haute-Provence Observatory. The new planet orbits HD 109246, a G0V star slightly more metallic than the Sun. HD 109246b has a minimum mass of 0.77 M(Jup), an orbital period of 68 days, and an eccentricity of 0.12. It is placed in a sparsely populated region of the period distribution of extrasolar planets. We also present a correction method for the so-called seeing effect that affects the SOPHIE radial velocities. We complement this discovery announcement with a description of some calibrations that are implemented in the SOPHIE automatic reduction pipeline. These calibrations allow the derivation of the photon-noise radial velocity uncertainty and some useful stellar properties (v sin i, [Fe/H], log R'(HK)) directly from the SOPHIE data.

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

4.6
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