Spectroscopic analysis of A- and F-type stars observed in the Kepler field

Magdalena Polińska, Ewa Niemczura, Simon J. Murphy, Hans Bruntt, Katrien Uytterhoeven and Peter De Cat

We present results obtained from a spectroscopic analysis of high-resolution spectra taken with the ESPADONS spectrograph at the Canada-France-Hawaii Telescope and the SOPHIE spectrograph installed at the telescope in Haute-Provence Observatory. The data were collected for A- and F-type stars observed in the Kepler field. The presented sample of stars consists of objects with the projected rotational velocities lower than 60 km s^-1. The atmospheric parameters, abundances and rotational velocities were calculated using the iSpec code with spectrum synthesis technique.

Proceedings of the Polish Astronomical Society, vol. 7, 197-200 (2018)

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