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Spectroscopic and Photometric Survey of Northern Sky for the ESA PLATO space mission

Published online by Cambridge University Press:  07 March 2018

Renata Ženovienė ,
Vilius Bagdonas ,
Arnas Drazdauskas ,
Rimvydas Janulis ,
Lukas Klebonas ,
Šarūnas Mikolaitis ,
Erika Pakštienė  and
Gražina Tautvaišienė
Renata Ženovienė
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: [email protected]
Vilius Bagdonas
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: [email protected]
Arnas Drazdauskas
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: [email protected]
Rimvydas Janulis
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: [email protected]
Lukas Klebonas
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: [email protected]
Šarūnas Mikolaitis
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: [email protected]
Erika Pakštienė
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: [email protected]
Gražina Tautvaišienė
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: [email protected]
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Abstract

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The ESA-PLATO 2.0 mission will perform an in-depth analysis of the large part of the sky-sphere searching for extraterrestrial telluric-like planets. At the Molėtai Astronomical Observatory of Vilnius University, we started a spectroscopic and photometric survey of the northern sky fields that potentially will be targeted by the PLATO mission. We aim to contribute in developing the PLATO input catalogue by delivering a long-duration stellar variability information and a full spectroscopic characterization of brightest targets. First results of this survey are overviewed.

Keywords

Stars:abundancesstars:oscillations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 283 - 284
Copyright
Copyright © International Astronomical Union 2018 

References

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