The discovery of a planetary candidate around the evolved low-mass Kepler giant star HD 175370
Journal article, 2017
stars: individual: HD 175370 (KIC 007940959)
methods: data analysis
techniques: radial velocities
methods: observational
techniques: spectroscopic
planetary systems
Author
M. Hrudkova
Isaac Newton Group
A. Hatzes
Thüringer Landessternwarte Tautenburg
R. Karjalainen
Isaac Newton Group
H. Lehmann
Thüringer Landessternwarte Tautenburg
S. Hekker
Max Planck Society
Aarhus University
M. Hartmann
Thüringer Landessternwarte Tautenburg
A. Tkachenko
KU Leuven
S. Prins
KU Leuven
H. van Winckel
KU Leuven
R. De Nutte
Royal Observatory of Belgium
L. Dumortier
Royal Observatory of Belgium
Y. Fremat
Royal Observatory of Belgium
H. Hensberge
Royal Observatory of Belgium
A. Jorissen
Université libre de Bruxelles (ULB)
P. Lampens
Royal Observatory of Belgium
M. Laverick
KU Leuven
Robin Lombaert
Chalmers, Earth and Space Sciences, Onsala Space Observatory
P. I. Papics
KU Leuven
G. Raskin
KU Leuven
A. Sodor
Royal Observatory of Belgium
Hungarian Academy of Sciences
A. Thoul
Kavli Institute for Theoretical Physics
University of Liège
S. Van Eck
Université libre de Bruxelles (ULB)
C. Waelkens
KU Leuven
Monthly Notices of the Royal Astronomical Society
0035-8711 (ISSN) 1365-2966 (eISSN)
Vol. 464 1 1018-1028Subject Categories
Astronomy, Astrophysics and Cosmology
DOI
10.1093/mnras/stw2379