Polińska, M. ; Niemczura, E. ; Murphy, S. J. ; Bruntt, H. ; Uytterhoeven, K. ; De Cat, P.

published in Proceedings of the Polish Astronomical Society, 7, pp. 197-200 (2018)

Abstract: 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.

Note: XXXVIII Polish Astronomical Society Meeting, Proceedings of the meeting held 11-14 September, 2017 in Zielona Góra, Poland
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