Alix V Freckelton
BEBOP V. Homogeneous stellar analysis of potential circumbinary planet hosts
Freckelton, Alix V; Sebastian, Daniel; Mortier, Annelies; Triaud, Amaury H M J; Maxted, Pierre F L; Acuña, Lorena; Armstrong, David J; Battley, Matthew P; Baycroft, Thomas A; Boisse, Isabelle; Bourrier, Vincent; Carmona, Andres; Coleman, Gavin A L; Cameron, Andrew Collier; Cortés-Zuleta, Pía; Delfosse, Xavier; Dransfield, Georgina; Duck, Alison; Forveille, Thierry; French, Jenni R; Hara, Nathan; Heidari, Neda; Hellier, Coel; Kunovac, Vedad; Martin, David V; Martioli, Eder; McCormac, James J; Nelson, Richard P; Sairam, Lalitha; Sousa, Sérgio G; Standing, Matthew R; Willett, Emma
Authors
Daniel Sebastian
Annelies Mortier
Amaury H M J Triaud
Pierre Maxted p.maxted@keele.ac.uk
Lorena Acuña
David J Armstrong
Matthew P Battley
Thomas A Baycroft
Isabelle Boisse
Vincent Bourrier
Andres Carmona
Gavin A L Coleman
Andrew Collier Cameron
Pía Cortés-Zuleta
Xavier Delfosse
Georgina Dransfield
Alison Duck
Thierry Forveille
Jenni R French
Nathan Hara
Neda Heidari
Coel Hellier c.hellier@keele.ac.uk
Vedad Kunovac
David V Martin
Eder Martioli
James J McCormac
Richard P Nelson
Lalitha Sairam
Sérgio G Sousa
Matthew R Standing
Emma Willett
Abstract
Planets orbiting binary systems are relatively unexplored compared to those around single stars. Detections of circumbinary planets and planetary systems offer a first detailed view into our understanding of circumbinary planet formation and dynamical evolution. The BEBOP (binaries escorted by orbiting planets) radial velocity survey plays a special role in this adventure as it focuses on eclipsing single-lined binaries with an FGK dwarf primary and M dwarf secondary allowing for the highest radial velocity precision using the HARPS and SOPHIE spectrographs. We obtained 4512 high-resolution spectra for the 179 targets in the BEBOP survey which we used to derive the stellar atmospheric parameters using both equivalent widths and spectral synthesis. We furthermore derive stellar masses, radii, and ages for all targets. With this work, we present the first homogeneous catalogue of precise stellar parameters for these eclipsing single-lined binaries.
Citation
Freckelton, A. V., Sebastian, D., Mortier, A., Triaud, A. H. M. J., Maxted, P. F. L., Acuña, L., …Willett, E. (2024). BEBOP V. Homogeneous stellar analysis of potential circumbinary planet hosts. Monthly Notices of the Royal Astronomical Society, 531(4), 4085-4098. https://doi.org/10.1093/mnras/stae1405
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 1, 2024 |
Online Publication Date | Jun 6, 2024 |
Publication Date | Jul 1, 2024 |
Deposit Date | Jul 17, 2024 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 531 |
Issue | 4 |
Pages | 4085-4098 |
DOI | https://doi.org/10.1093/mnras/stae1405 |
Keywords | techniques: spectroscopic, binaries: eclipsing, binaries: spectroscopic |
Public URL | https://keele-repository.worktribe.com/output/859588 |
Publisher URL | https://academic.oup.com/mnras/article/531/4/4085/7689218?login=true#467520866 |
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