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

Bibcode
2018pas7.conf..197P
Polińska, Magdalena; Niemczura, Ewa; Murphy, Simon J.; Bruntt, Hans; Uytterhoeven, Katrien; De Cat, Peter
Bibliographical reference

XXXVIII Polish Astronomical Society Meeting, Proceedings of the meeting held 11-14 September, 2017 in Zielona Góra, Poland. Proceedings of the Polish Astronomical Society, Vol. 7, Edited by Agata Różańska. ISBN: 978-83-950430-0-0, 2018, pp.197-200

Advertised on:
8
2018
Number of authors
6
IAC number of authors
1
Citations
0
Refereed citations
0
Description
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.
Type
Non-refereed

It may interest you

  • Non-refereed
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Advertised on:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Citations
    0
  • Non-refereed
    The Multi Frequency Instrument 2 (MFI2): mechanical design, manufacture, integration, and commissioning of the MFI2 for the QUIJOTE facility in Tenerife (Canary Islands)
    The QUIJOTE (Q-U-I JOint TEnerife) experiment combines the operation of two radio-telescopes and three instruments working in the microwave bands from 10 to 47 GHz at the Teide Observatory, Tenerife, which has already been presented in previous SPIE meetings. The new Multi Frequency Instrument (MFI2) led by the Instituto de Astrofísica de Canarias
    Lorenzo-Hernández, Haroldo et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..33L
    Citations
    0
  • Non-refereed
    ANDES, the high-resolution spectrograph for the ELT: RIZ & UBV spectrographs' preliminary design, analysis, and integration of the vacuum vessel and thermal enclosure
    The RIZ & UBV visible spectrographs of the ANDES instrument, which are foreseen to be installed at the Extremely Large Telescope, require to be under a very stable high vacuum and at an extremely stable temperature of 1mK to reach the radial velocity goal of 10cm/s RMS over a 10-year period. The baseline design, integration and first analyses of
    Santos Diaz, P. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..4KS
    Citations
    0