Evidence for an additional planet in the β Pictoris system (original) (raw)
Data availability
The HARPS spectra are available in the ESO archive, and the measured RV data are given in Supplementary Table 1.
Code availability
The codes used for this paper are available from the corresponding author upon reasonable request.
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Acknowledgements
This work has been supported by grants from the Agence Nationale de la Recherche (ANR-14-CE33–0018) and the French Labex OSUG@2020 (Investissements d’avenir—ANR10 LABX56). A.Z. was supported by CONICYT grant no. 2117053. A.-M.L. thanks F. Forbes, K. Zwincks, A. Lecavelier, J. Pepper, P. Kervella and J. C. B. Papaloizou for discussions. T.G., D.M., L.A. and F.-X.S. acknowledge support from Idex UCAJEDI (ANR-15-IDEX-01) and IPEV.
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Authors and Affiliations
- Institut de Planétologie et d’Astrophysique de Grenoble, Université Grenoble Alpes, CNRS, IPAG, Grenoble, France
A.-M. Lagrange, Nadège Meunier, Miriam Keppler, Franck Galland, Hervé Beust, Antoine Grandjean, Simon Borgniet, Mickael Bonnefoy & Laetitia Rodet - Pixyl, La Tronche, France
Pascal Rubini - Max Planck Institute for Astronomy, Heidelberg, Germany
Miriam Keppler - Université Côte d’Azur, OCA, Lagrange CNRS, Nice, France
Eric Chapellier, Tristan Guillot, Djamel Mékarnia, Lyu Abe & François-Xavier Schmider - LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France
Eric Michel - South African Astronomical Observatory, Cape Town, South Africa
Luis Balona - CNRS, UMR7095, Institut d’Astrophysique de Paris, Paris, France
Paul Anthony Wilson & Flavien Kiefer - Department of Physics, University of Warwick, Coventry, UK
Paul Anthony Wilson - Leiden Observatory, Leiden University, Leiden, the Netherlands
Paul Anthony Wilson - European Southern Observatory, Vitacura, Santiago, Chile
Jorge Lillo-Box, Blake Pantoja & Matias Jones - Departamento de Astronomía, Universidad de Chile, Las Condes, Santiago, Chile
Blake Pantoja & Matias Diaz - Instituto de Fisica y Astronomia, Facultad de Ciencias, Universidad de Valparaíso, Valparaíso, Chile
Daniela Paz Iglesias - Núcleo Milenio de Formación Planetaria—NPF, Universidad de Valparaíso, Valparaíso, Chile
Daniela Paz Iglesias - Center of Astro-Engineering, Department of Electrical Engineering, Pontificia Universidad Catolica de Chile, Santiago, Chile
Abner Zapata
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Contributions
A.-M.L. led the monitoring of the variations, the data reduction, the analysis and interpretation of the data, and the paper writing. N.M., P.R., M.K. and F.G. participated to the data fitting and analysis. E.C., E.M., L.B. and F.-X.S. brought their expertise in stellar variability. H.B. provided analysis of the dynamical stability of the system. T.G., D.M. and L.A. brought expertise on β Pictoris photometric variability. P.A.W. and F.K. brought expertise on β Pictoris spectroscopic variability. M.B., S.B., A.G., J.L.-B., B.P., D.P.I., L.R. and A.Z.S. participated in the observations.
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Correspondence toA.-M. Lagrange.
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Lagrange, AM., Meunier, N., Rubini, P. et al. Evidence for an additional planet in the β Pictoris system.Nat Astron 3, 1135–1142 (2019). https://doi.org/10.1038/s41550-019-0857-1
- Received: 22 October 2018
- Accepted: 04 July 2019
- Published: 19 August 2019
- Issue Date: December 2019
- DOI: https://doi.org/10.1038/s41550-019-0857-1