Yveline Lebreton
- Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA)
- Institut de Physique de Rennes (IPR)
- Laboratoire d’Instrumentation et de Recherche en Astrophysique (LIRA)
- Étoiles et Galaxies
Présentation
Publications
Publications
Stellar science core program of the PLATO missionAnnual meeting of the European Astronomical Society, Session SS1a: SS1a: PLATO's Prospects in Exoplanet and Stellar Science, European Astronomical Society, Jun 2025, Cork (Irlande), Ireland |
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Stellar age-datingGalactic Archeology kick-off meeting, Jun 2024, Meudon, France |
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The CESAM2K20 stellar evolution codeJournées 2024 de la Société Française d’Astronomie & d’Astrophysique (SF2A 2024), Jun 2024, Marseille, France. pp.467-471 |
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A selection of astrometric binaries from GAIA-DR3 that could be double-lined spectroscopic binaries and eclipsing binariesSF2A 2023, May 2023, Strasboug, France |
Hare&Hounds Exercise for Stellar Ages Hare&Hounds Exercise for Stellar Ages and Masses in the Context of FGK Stars and Masses in the Context of FGK Stars with and without Asteroseismology. with and without AsteroseismologyPLATO Stellar Science Conference 2023, held 26-30 June 2023, in Milazzo (Italy)., Jun 2023, Milazzo, Italy. ⟨10.5281/zenodo.8117392⟩ |
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Masses and luminosities of SB2 components deduced from OHP spectroscopic observations and GAIA-DR3 astrometric orbitsSF2A 2023, May 2023, Strasbourg, France |
Some inputs and developments of CestamCesam Workshop, Jun 2022, Meudon, France |
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The SPInS's pipeline for stellar properties inferenceGalactic Archeology, Mar 2021, Birmingham, United Kingdom |
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Magnetism and Accretion in Intermediate-Mass PMS StarsA Workshop in Honour of the Career and Contributions of John D. Landstreet, Gregg Wade (chief editor), Evelyne Alecian, David Bohlender, Aaron Sigut, Jul 2019, London, Canada. pp.125 |
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From the star to the transiting exoplanets: Characterisation of the HD 219134 systemSF2A 2019, May 2019, NICE, France |
The Hertzsprung-Russell diagramme in the Gaia Era.In 5th International Yound Astronomer School: Scientific Exploita tion of the Gaia Data, Paris, Feb 2018, Paris, France |
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Mass, radius, and composition of the transiting planet 55 Cnc e : using interferometry and correlationsSF2A Week, Jul 2018, Bordeaux, France |
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Asteroseismology of solar-like stars'How Much do we Trust Stellar Models?', held in Liège (Belgium), 10-12 September 2018, Sep 2018, Liège, Belgium |
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Bilan des activités du PNPS/INSU sur la période 2014-2018Colloque de prospective du PNPS, Methode et objec- tifs, Montpellier Mars 2018., Mar 2018, Montpellier, France |
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The programme: Accurate masses for double-lined spectroscopic binary componentsPLATO STESCI WORKshop ii, May 2018, Milazzo, Italy |
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Hands-on exercises: Stellar age determination.In 5th International Yound Astronomer School: Scientific Exploitation of the Gaia Data, Paris, Feb 2018, Paris, France |
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Current updated grids of 1D stellar models: Cestam mockgrid.PLATO SPC WP120 2017 meeting, May 2017, Liège, Belgium |
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Low mass stars stellar models: a roadmap for WP121120.PLATO SPC WP120 2017 meeting, May 2017, Liège, Belgium |
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The programme ``accurate masses for SB2 componentsSF2A Week, Jul 2017, Paris, France |
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Stellar models and their limitations: Three questions on stellar modelsSymposium Ages2: Taking Stellar Ages to the Next Power,, Sep 2017, Isola Elba, Italy |
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Automatic search for optimal models using Levenberg-Marquardt algorithmPLATO WP120 2016 Meeting, May 2016, Meudon, France |
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An attempt to calibrate core overshooting using the seismic properties of low-mass starsThe Space Photometry Revolution - CoRoT Symposium 3, Kepler KASC-7 Joint Meeting, Jul 2014, Toulouse, France. pp.id.01013, ⟨10.1051/epjconf/201510101013⟩ |
Accurate stellar masses for SB2 components: Interferometric observations for Gaia validationSF2A-2015: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, Jun 2015, Toulouse, France. pp.377 - 380 |
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An attempt to calibrate core overshooting using the seismic properties of low-mass starsThe Space Photometry Revolution - CoRoT Symposium 3, Kepler KASC-8, Jul 2015, Toulouse, France, France |
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Derivation of the mass ratios of 20 new double-lined spectroscopic binariesSemaine de l'Astrophysique, SF2A 2014, Jun 2014, Paris, France. pp.159 - 161 |
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The programme "accurate masses for SB2 componentsSemaine de l'Astrophysique, SF2A 2014, Jun 2014, Paris, France. pp.427 - 430 |
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Impact of asteroseismology on improving stellar ages determinationNew Advances in Stellar Physics: From Microscopic to Macroscopic Processes, May 2013, Roscoff, France. ⟨10.1051/eas/1363014⟩ |
Improved SB2 orbits for HIP 12081 and HIP 87895Semaine de l'Astrophysique, SF2A 2013, Jun 2013, Montpellier, France. pp.127 - 135 |
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Seismic Ages of StarsERC Symposium, What asteroseismology has to offer to astrophysics, Dec 2013, Brussels, Belgium |
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Transport of angular momentum in solar-like oscillating starsPrecision Asteroseismology, Proceedings of the International Astronomical Union, IAU Symposium, Volume 301, pp. 161-168, Aug 2013, Wrocław, Poland. ⟨10.1017/S1743921313014269⟩ |
Seismic Ages of StarsFRANQUI ERC Symposium, What Asteroseismology has to offer to Astrophysics, Dec 2013, Bruxelles, Belgium |
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A new method based on Markov chains for deriving SB2 orbits directly from their spectraCongrès de la Société Française d'Astronomie et d'Astrophysique, Jun 2012, Nice, France |
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Ages of Exoplanet Host-Stars from Asteroseismology61st Fujihara Seminar "Progress in Solar / Stellar Physics with Helio- and Asteroseismology", Mar 2011, Hakone, Japan. pp.469 |
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New SB2 orbital elements for accurate masses with Gaia: HD 9312, HD 9313 and HD 183255Semaine de l'Astrophysique, SF2A 2012, Jun 2012, Nice, France. pp.87 - 90 |
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Age dating large samples of stars: the Gaia contextCongrès de la Société Française d'Astronomie et d'Astrophysique, Jun 2012, Nice, France |
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Modèles stellaires 1D : État de l'artColloque de clôture de l'ANR ESTER, 2012, Toulouse, France |
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Stellar age determination through asteroseismologySemaine de l'Astrophysique, SF2A 2012, Jun 2012, Nice, France |
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Age dating large samples of stars: ways toward improved accuracyCongrès de la Société Française d'Astronomie et d'Astrophysique, Jun 2012, Nice, France |
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Stellar age-dating for different Gaia simulated catalogs"Stellar Populations 55 years after the Vatican Conference",, Jul 2012, Rome, Italy |
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Stellar age determination through asteroseismologySemaine de la SF2A 2012, Jun 2012, Nice, France, France |
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A new method based on Markov chains for deriving SB2 orbits directly from their spectraSF2A-2012: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, Jun 2012, Nice, France, France. pp.117-120 |
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Open issues in probing interiors of solar-like oscillating main sequence stars: 2. Diversity in the HR diagramGONG–SoHO 24: A new era of seismology of the sun and solar-like stars, Jun 2010, Aix-en-Provence, France. ⟨10.1088/1742-6596/271/1/012032⟩ |
Determination of the ages of stars from their position in the HR diagramSemaine de l'Astrophysique, SF2A 2011, Jun 2011, Paris, France. pp.295 - 298 |
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New SB2 binaries for accurate stellar masses with GaiaSemaine de l'Astrophysique, SF2A 2011, Jun 2011, Paris, France. pp.303 - 306 |
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Stellar Age DeterminationPLATO SSPM Meeting, Jan 2011, Paris, France |
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Open issues in probing interiors of solar-like oscillating main sequence stars 1. From the Sun to nearly sunsGONG–SoHO 24: A new era of seismology of the sun and solar-like stars, Jun 2010, Aix-en-Provence, France. ⟨10.1088/1742-6596/271/1/012031⟩ |
Ages of Exoplanet Host-stars from Asteroseismology: HD 17156, a Case StudyThe 61st Fujihara seminar: Progress in solar/stellar physics with helio- and asteroseismology", Mar 2011, Fujoihara, Japan |
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New Perspectives in Stellar Physics: Gaia in the 2015 contextGAIA: At the Frontiers of Astrometry, Jun 2010, Sèvres, France. pp.245, ⟨10.1051/eas/1045041⟩ |
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Comparisons between stellar models and reliability of the theoretical modelsSynergies between solar and stellar modelling, Jun 2010, Rome, Italy. ⟨10.1007/s10509-010-0314-1⟩ |
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Stellar ages from asteroseismologyThe Ages of Stars, IAU Symposium 258, Oct 2008, Baltimore, MD, United States, United States. pp.419-430 |
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CoRot observations of active giants: preliminary resultsCOOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, Jul 2008, St. Andrews (Scotland), United Kingdom. pp.864-867, ⟨10.1063/1.3099253⟩ |
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Stars in the age of micro-arc-second astrometryA Giant Step: from Milli- to Micro-arcsecond Astrometry, IAU Symposium 248, Oct 2007, Shanghai, China, Nanjing, China. pp.411-416, ⟨10.1017/S1743921308019728⟩ |
Calibration of the Pre Main Sequence Binary System RS Cha: Impact of the Initial Chemical MixtureBinary Stars as Critical Tools and Tests in Contemporary Astrophysics http://ad.usno.navy.mil/iaus240/, IAU Symposium 240, Aug 2006, Prague, Czech Republic, Czech Republic. pp.385 |
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Calibration of the Pre-Main Sequence Binary System RS Cha: Impact of the Initial Chemical MixtureBinary Stars as Critical Tools and Tests in Contemporary Astrophysics http://ad.usno.navy.mil/iaus240/, IAU Symposium 240, Aug 2006, Prague, Czech Republic, Czech Republic. pp.652-657, ⟨10.1017/S1743921307006059⟩ |
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Comparisons for ESTA-Task3: CLES and CESAMStellar Evolution and Seismic Tools for Asteroseismology - Diffusive Processes in Stars and Seismic Analysis, Nov 2006, Porto, Portugal. pp.167-176, ⟨10.1051/eas:2007135⟩ |
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Asteroseismology of delta Scuti stars in open clusters: PraesepeProceedings of the Vienna Workshop on the Future of Asteroseismology, 2007, Vienna, Austria. pp.39-43, ⟨10.1553/cia151s39⟩ |
RS Cha, a spectroscopic binary system as a test of stellar physics modeling during the pre-main sequence phaseSF2A-2005: Semaine de l'Astrophysique Francaise, Jun 2005, Strasbourg, France, France. pp.299 |
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Preliminary numerical effects of shellular rotation on adiabatic frequenciesStellar Structure and Habitable Planet Finding, Apr 2003, Palermo, Italy. pp.431-434 |
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Effect of Local Treatments of Convection upon the Solar P-Mode Excitation RatesSOHO 14 Helio- and Asteroseismology: Towards a Golden Future, Jul 2004, Haven, Connecticut, United States. pp.611 |
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ENEAS: the European Network of Excellence in AsteroSeismologyStellar Structure and Habitable Planet Finding, Apr 2003, Palermo, Italy. pp.247-250 |
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Application of New ATLAS9 Model Atmosphere GridsModelling of Stellar Atmospheres, IAU Symposium 210, Jun 2002, Uppsala, Sweden, Sweden |
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Oscillation power across the H-R diagram: sensitivity to the convection treatmentStellar Structure and Habitable Planet Finding, Jun 2001, Córdoba, Spain. pp.87-94 |
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GAIA and Physics of Stellar InteriorsGAIA: A European Space Project, May 2001, Les Houches, France. pp.131-144 |
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Cepheids in the SMC: Blue Loops and Mass-Luminosity RelationObserved HR Diagrams and Stellar Evolution, Jun 2001, Coimbra, Portugal, Portugal. pp.69 |
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A Study of Convection with delta Scuti Stars in Open Clusters: the PleiadesIAU Colloq. 185: Radial and Nonradial Pulsationsn as Probes of Stellar Physics, Jul 2001, Leuven, Belgium, Belgium. pp.490 |
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Seismology of delta Scuti stars in open clustersSF2A-2002: Semaine de l'Astrophysique Francaise, Jun 2002, Paris, France, France. pp.569 |
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Analysis of Seven Nearby Open Clusters using HIPPARCOS DataSymposium 'Hipparcos - Venice 97', May 1997, Venice, Italy |
Project of a Knowledge Base for Internal StructureArtificial Intelligence Techniques for Astronomy, 1990, Strasbourg, France |
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Surface Abundances of Light Elements as Diagnostic of Transport Processes in the Sun and Solar-Type StarsInside the Sun, Proceedings of IAU Colloq. 121, 1989, Versailles, France. ⟨10.1007/978-94-009-0541-2_39⟩ |
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Project of a knowledge base for internal structure.Artificial Intelligence Techniques in Astronomy, 1989, Paris, France |
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The influence of the equation of state on the zero-age main sequence and the SunESA, Seismology of the Sun and Sun-Like Stars, Sep 1988, Puerto de La Cruz, Spain |
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Solar neutrinos, solar oscillations and turbulent diffusion mixingAdvances in nuclear astrophysics; Proceedings of the Second IAP Workshop, Paris, France, July 7-11, Jul 1986, Paris, France |
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A Solar Model with Turbulent Diffusion Mixing - Surface Abundances and OscillationsAdvances in Helio- and Asteroseismology, Proceedings of the Symposium held 17-11 July 1986, in Aarhus, Denmark., Jul 1986, Aarhus, Denmark |
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Solar neutrinos, solar oscillations and turbulent diffusion mixingAdvances in nuclear astrophysics, Second IAP Workshop, Paris, France, Jul 1986, Paris, France. pp.105 - 110 |
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A Solar Model with Turbulent Diffusion Mixing - Surface Abundances and OscillationsAdvances in Helio- and Asteroseismology,, J. Christensen-Dalsgaard and S. Frandsen, Jul 1986, Aarhus (Danemark), Denmark. pp.95 |
Stellar age-dating for different Gaia simulated catalogsA. Omizzolo, M. Fabrizio, G. Bono. STELLAR POPULATIONS 55 YEARS AFTER THE VATICAN CONFERENCE, Jul 2012, Rome, Italy. 86, pp.342, 2012, Memorie della Societa Astronomica Italiana |
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Stellar Age-dating for different Gaia simulated catalogsEWASS Symposium 6 "Stellar Populations 55 years after the Vatican Conference", Jul 2012, Rome, Italy |
Multi-Dimensional Processes In Stellar Physics2020 |
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Imaging at High Angular Resolution of Stellar Surfaces and Close Environment2019 |
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Foreword80-81, pp.1 - 3, 2016, ⟨10.1051/eas/1680001⟩ |
Stellar Clusters: Benchmarks of Stellar Physics and Galactic Evolution - EES201580, 2016 |
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Preface to: The Ages of Stars65, 2014, ⟨10.1051/eas/1465000⟩ |
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Preface to: New Advances in Stellar Physics: From Microscopic to Macroscopic Processes63, 2013, ⟨10.1051/eas/1363000⟩ |
New Advances in Stellar Physics: From Microscopic to Macroscopic Processes2013 |
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Oxygen in the UniverseEDP Sciences, 54, 370 p., 2012, EAS Publications Series |
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How accurate are stellar ages based on stellar models? II. The impact of asteroseismologyThe age of stars, 65, pp.177 - 223, 2014, EAS Publications Series, ⟨10.1051/eas/1465005⟩ |
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How accurate are stellar ages based on stellar models? I. The impact of stellar models uncertaintiesThe Ages of Stars, 65, pp.99-176, 2014, EAS Publications Series, ⟨10.1051/eas/1465004⟩ |
Chapter 2 : A Panorama of Oxygen in the UniverseOxygen in the Universe, 54, 2012, ⟨10.1051/eas/1254002⟩ |
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Solar interior modelsSolar interior and atmosphere, 1991 |
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The surface composition of six newly discovered chemically peculiar stars. Comparison to the HgMn stars $\mu$ Lep and $\beta$ Scl and the superficially normal B star $\nu$ Cap2023 |
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Gaia Data Release 3: Chemical cartography of the Milky Way2022 |
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Gaia Data Release 3: Reflectance spectra of Solar System small bodies2022 |
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Gaia Data Release 3: Chemical cartography of the Milky Way2022 |
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The Aarhus Red Giants Challenge I: Stellar structures in the red giant branch phase2019 |
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The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition[Research Report] MSE Science Team. 2019 |
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Star-Planet InteractionsEvry Schatzman School 2019, Sep 2019, Aussois (France), France. EDP Sciences, 2023, 9782759831548. ⟨10.1051/978-2-7598-3154-8⟩ |