SAC Seminar - Suba Dong: Kepler Planet Census Aided by LAMOST

2018.03.02 | Louise Børsen-Koch

Date Fri 09 Mar
Time 14:15 15:00
Location 1520-616

The lack of spectroscopic stellar parameters for the majority of Kepler target stars present a major limitation to Kepler planet statistics. An ongoing spectroscopic survey of the Kepler field has been conducted by the LAMOST telescope in China, and accurate stellar parameters have already been obtained for tens of thousands of Kepler targets. I discuss recent studies using the LAMOST data that lead to new insights into our understanding of Kepler planet distributions.

Public/media, Staff, Students