2nd LAMOST-Kepler workshop

OAN-SPM spectroscopic observations of a number of stars in the Kepler field: Comparison with LAMOST database.

1 Aug 2017, 10:20

20m

Meridian Room (Royal Observatory of Belgium)

Contributed talk 2.2 The LAMOST as a large spectroscopic survey 2.2 The LAMOST as a large spectroscopic survey

Speaker

Dr Lester Fox-Machado (Instituto de Astronomia-Universidad Nacional Autonoma de Mexico (UNAM))

Description

We present low and medium resolution spectroscopy of a number of stars in the kepler-field-of-view obtained in the past few years during several runs at the Observatorio Astronomico Nacional-San Pedro Martir (OAN-SPM) in Baja California, Mexico. The Boller & Chivens spectrograph installed in the Cassegrain focus of the 2.12-m telescope has been used. The atmospheric parameters of the stars have been computed using the iSpec tool for the analysis of stellar spectra (Blanco-Cuaresma et al. 2014). A comparison between derived physical parameters and those listed in the LAMOST public database is presented.

Presentation materials

Slides

17lamost_Presentation_CT03_FoxMachadoLester.pdf