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BEBOP VI. enabling the detection of circumbinary planets orbiting double-lined binaries with the DOLBY method of radial-velocity extraction

Sairam, Lalitha; Baycroft, Thomas A; Boisse, Isabelle; Heidari, Neda; Santerne, Alexandre; Triaud, Amaury H M J; Coleman, Gavin A L; Davis, Yasmin T; Deleuil, Magali; Hébrard, Guillaume; Martin, David V; Maxted, Pierre F L; Nelson, Richard P; Sebastian, Daniel; Scutt, Owen J; Standing, Matthew R

Authors

Lalitha Sairam

Thomas A Baycroft

Isabelle Boisse

Neda Heidari

Alexandre Santerne

Amaury H M J Triaud

Gavin A L Coleman

Yasmin T Davis

Magali Deleuil

Guillaume Hébrard

David V Martin

Richard P Nelson

Daniel Sebastian

Owen J Scutt

Matthew R Standing



Abstract

Circumbinary planets, orbiting both stars in a binary system, offer the opportunity to study planet formation and orbital migration in an environment different from that around single stars. However, despite the fact that $> 90~{{\%}}$ of binary systems in the solar neighbourhood are spectrally resolved double-lined binaries, there has been only one detection of a circumbinary planet orbiting a double-lined binary using the radial velocity method so far. Spectrally disentangling binary components is challenging due to blending of spectral lines and inaccuracies in spectral modeling. These inaccuracies adds scatter to the measurements, which can hide the weak radial-velocity signature of circumbinary exoplanets. We have obtained new high signal-to-noise, high-resolution spectra with the SOPHIE spectrograph, mounted on the 193cm telescope at Observatoire de Haute-Provence (OHP), for six bright, double-lined binaries for which circumbinary exoplanet detection has been attempted in the past. To extract radial velocities, we use the DOLBY code, a recent method of spectral disentangling using Gaussian processes to model the time-varying components. We analyse the resulting radial-velocities with a diffusive nested sampler to seek planets, and compute sensitivity limits. We do not detect any new circumbinary planet. However, we show that the combination of new data, new radial velocity extraction methods, and improved statistical methods to determine a dataset’s sensitivity to planets leads to an approximately one order of magnitude improvement compared to previous results. This improvement brings us into the range of known circumbinary exoplanets and paves the way for future observation campaigns targeting double-lined binaries.

Citation

Sairam, L., Baycroft, T. A., Boisse, I., Heidari, N., Santerne, A., Triaud, A. H. M. J., …Standing, M. R. (in press). BEBOP VI. enabling the detection of circumbinary planets orbiting double-lined binaries with the DOLBY method of radial-velocity extraction. Monthly Notices of the Royal Astronomical Society, 534(4), 3999-4017. https://doi.org/10.1093/mnras/stae2317

Journal Article Type Article
Acceptance Date Oct 3, 2024
Online Publication Date Oct 10, 2024
Deposit Date Nov 8, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 534
Issue 4
Pages 3999-4017
DOI https://doi.org/10.1093/mnras/stae2317
Keywords techniques: radial velocities, techniques: spectroscopic - planets and satellites: detection, binaries: spectroscopic
Public URL https://keele-repository.worktribe.com/output/955551
Publisher URL https://academic.oup.com/mnras/article/534/4/3999/7817980