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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

Alix V Freckelton

Daniel Sebastian

Annelies Mortier

Amaury H M J Triaud

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

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