2nd LAMOST-Kepler workshop

Session

2.3 The LAMOST as a large spectroscopic survey

2.3

1 Aug 2017, 11:30

Meridian Room (Royal Observatory of Belgium)

Description

Ground-based support for space missions

55. LAMOST as a ground-based support facility for the space missions

Prof. JIANNING FU (BEIJING NORMAL UNIVESITY)

01/08/2017, 11:30

2.3 The LAMOST as a large spectroscopic survey

Invited Review

In the era of space missions such as Kepler and K2 which can provide extremely high duty-cycle, high-precision time-series photometric observations for a large number of stars in multiple stellar populations, ground-based spectroscopic observations are needed to characterize hundreds of thousands of stars in a homogeneous way, to support the research of exoplanets, asteroseismology, Galactic...

60. Analysis of the stellar parameters based on the LAMOST-K2 project data

Mrs Ruyuan Zhang (Beijing normal university)

01/08/2017, 12:10

2.3 The LAMOST as a large spectroscopic survey

Invited talk

Massive photometric data of different parts of the galaxy were obtained by covering 16 campaigns around the eclipse through K2, the second phase of the Kepler mission. Unlike the Kepler space telescope K2 mainly focuses on the data of more bright stars. Applying the ground based survey it is way more competent to observe those bright stars. LAMOST, a very influential ground based facility...

56. Asteroseismic analysis of selected High Amplitude Delta Scuti Candidates in the Kepler field

Dr Ceren Ulusoy (1.Girne American University, University Drive, PO Box 5, 99428 Karmi Campus, Karaoğlanoğlu, Kyrenia, Turkey 2.College of Graduate Studies, University of South Africa, PO Box 392, Unisa, 0003, Pretoria, South Africa)

01/08/2017, 12:40

2.3 The LAMOST as a large spectroscopic survey

Contributed talk

We present preliminary results on the analysis of the *Kepler* light curve of selected HADS candidates. Initially, *Kepler* data are used to derive frequency content of the variability of the stars. Then, the frequency analysis has been performed for each star using the software package SigSpeC (Reegen, 2007). The period ratios for the modes of highest amplitude are therefore discussed in the...