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Monday 11 October  |
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| Time (CEST) | Title | Speaker | Affiliation | |
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PLATO Mission (Chair: Isabella Pagano) |
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| 14:00 | Welcome and introduction | |
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| 14:10 |
The PLATO mission: Definition and status |
PLATO Team members |
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PLATO science objectives - PLATO Mission Consortium |
Heike Rauer |
DLR |
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Consortium scientific activities and community involvement |
Don Pollacco |
U. Warwick |
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PLATO mission design, spacecraft and payload |
Filippo Marliani Frank Steier Luca Valenziano Gisbert Peter |
ESA OHB INAF DLR |
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PLATO Ground Segment - an overview |
Laurence O'Rourke Laurent Gizon |
ESA MPS |
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PLATO as a resource for the astronomical community |
Ana Heras |
ESA |
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| 15:30 | Coffee Break | |||
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PLATO skyfields and PIC (Chair: Keivan Stassun) |
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| 15:45 | The PLATO Input Catalogue and Sky field selection | Giampaolo Piotto | Università degli Studi di Padova | |
| 16:15 | The TESS Input Catalog and Lessons For PLATO (invited) | Joshua Pepper | Lehigh University | |
| 16:45 | CARMENES and the Frontiers of High-Resolution Spectroscopy for M dwarfs: Fundamental Stellar Parameters and Chemical Abundances | Yutong Shan | University of Göttingen | |
| 17:00 | Discussion | |||
| 17:30 | Coffee Break | |||
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Planetary structure, composition, evolution and architecture of planetary systems (i) (Chair: Andrew Winter) |
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| 17:45 | New insights into Super-Earth interiors (invited) | Caroline Dorn | University of Zurich | |
| 18:15 | Characterisation of the interior structures and atmospheres of multiplanetary systems. | Lorena Acuña | LAM | |
| 18:30 | On the origin of the radius valley: formation and evolution | Christoph Mordasini | University of Bern | |
| 18:45 | Exploring the Nu2 Lupi system with CHEOPS | Laetitia Delrez | University of Liege | |
| 19:00 | Transit-Radial Velocity synergy to unveil the young exoplanet population and study the evolution of planetary systems | Serena Benatti | INAF - Astronomical Observatory of Palermo | |
| 19:15 | End of Day 1 | |||
Pre-recorded Talks |
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| Tidal dissipation in stars and predictions for planetary orbital decay | Adrian Barker | University of Leeds | |
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| Kepler-93: a testbed for detailed seismic modelling and orbital evolution of super-earths around solar-like stars | Jérôme Bétrisey | Université de Genève | |
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| Nonzero eccentricities of warm Neptunes | Alexandre Correia | University of Coimbra | |
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| Synthetic Evolution Tracks of Giant Planets | Simon Müller | Institute for Computational Science, University of Zurich | |
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| Tuesday 12 October |
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| Time (CEST) | Title | Speaker | Affiliation | |
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Planetary structure, composition, evolution and architecture of planetary systems (ii) (Chair: Cilia Damiani ) |
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| 14:00 | Correlations in Planetary System Architecture | Lokesh Mishra | University of Geneva and Bern | |
| 14:15 | CHEOPS and HARPS characterisation of a multi-planet system discovered by TESS | Thomas Wilson | University of St Andrews | |
| 14:30 | Stability and spacing of tightly packed systems | Antoine Petit | University of Copenhagen | |
| 14:45 | Extreme exoplanet obliquities due to the tidal migration of unseen moons | Melaine Saillenfest | IMCCE, Observatoire de Paris | |
| 15:00 | Chemical abundances of stars and their impact on the interior structure of rocky planets (invited) | Natalie Hinkel | Southwest Research Institute | |
| 15:30 | Coffee Break | |||
| 15:45 | Unveiling the atmospheric evolution of exoplanets | Andrea Bonfanti | ÖAW - Austrian Academy of Sciences | |
| 16:00 | Poster pitch presentations | |||
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Asteroseismology and stellar characterisation (Chair: Gaël Buldgen) |
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| 16:15 | Asteroseismic Data Analysis for Mode Frequencies for PLATO (invited) | Guy Davies | University of Birmingham | |
| 16:45 | Seismic modeling of solar-like pulsators in the PLATO era (invited) | Sebastien Deheuvels | Institut de Recherche en Astrophysique et Planétologie | |
| 17:15 | PLATO Hare-and-Hounds exercise: Modelling main sequence stars | Margarida Cunha | Instituto de Astrofísica e Ciências do Espaço | |
| 17:30 | Coffee Break | |||
| 17:45 | Asteroseismic probing of low mass solar-like stars throughout their evolution with new techniques | Martin Farnir | Université de Liège | |
| 18:00 | Non-seismic (and Non-LTE) stellar parameters for the PLATO core sample (invited) | Maria Bergemann | Max Planck Institute for Astronomy DE | |
| 18:30 | What to expect from non-seismic stellar characterisation with PLATO lightcurves | Lisa Bugnet | Center for Computational Astrophysics, Flatiron Institute | |
| 18:45 | Asteroseismic measurement of the inclination angle: characterizing exoplanetary systems | Charlotte Gehan | Max Planck Institute for Solar System Research | |
| 19:00 | Simultaneous seismic modelling of multiple stars using correlated parameters | Warrick Ball | University of Birmingham | |
| 19:15 | End of Day 2 | |||
Pre-recorded Talks |
| Characterization of 12 TESS Exoplanet Hosts with Solar-like Oscillations | Bernardo Ferreira | Universidade Federal de Minas Gerais | |
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| Wednesday 13 October |
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| Time (CEST) | Title | Speaker | Affiliation | |
| Stellar variability (Chair: Timo Reinhold ) | ||||
| 14:00 | Characterising small exoplanets in the face of intrinsic stellar variability (invited) | Raphaelle Haywood | University of Exeter | |
| 14:30 | Evolution of magnetic activity on the main sequence as a function of spectral type using Kepler data | Savita Mathur | Instituto de AstrofÍsica de Canarias | |
| 14:45 | Rotation & activity of M dwarfs: From K2 to TESS and PLATO | Beate Stelzer | Eberhard-Karls Universität Tübingen | |
| 15:00 | Seismic diagnostics of stellar activity cycles | Valeriy Vasilyev | Max Planck Institute for Solar System Research | |
| 15:15 | Characterizing stellar granulation with 3D stellar atmosphere models | Luisa Fernanda Rodríguez Díaz | Stellar Astrophysics Centre, Aarhus University | |
| 15:30 | Coffee Break | |||
| 15:45 | Poster pitch presentations | |||
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Long-period small planets and habitability (Chair: Tim Lichtenberg ) |
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| 16:00 | Terrestrial Exoplanet Habitability and Characterization: Opportu- nities and Challenges (invited) | Victoria Meadows | University of Washington | |
| 16:30 | Water oceans on high-density exoplanets from coupled interior-atmosphere modeling | Philipp Baumeister | DLR Berlin | |
| 16:45 | Kepler’s Small Planets and their Dependence on Stellar Mass | Galen Bergsten | Lunar and Planetary Laboratory, The University of Arizona | |
| 17:00 | Eta-Earth Revisited: A Formula for Earth-like Habitats | Helmut Lammer | Austrian Academy of Sciences, Space Research Institute | |
| 17:15 | HIP41378: a foretaste of PLATO | Alexandre Santerne | Laboratoire d'Astrophysique de Marseille | |
| 17:30 | Coffee Break | |||
| 17:45 | The Consequences of Binary Exoplanet Host Stars | Steve Howell | NASA | |
| 18:00 | Planets are places: Characterization of other Worlds in the 2020s and Beyond (invited) | Laura Kreidberg | Max Planck Institute for Astronomy DE | |
| 18:30 | Habitability and loss of hydrogen-helium atmospheres of small planets - the K dwarf advantage |
Katja Poppenhäger | Leibniz Institute for Astrophysics Potsdam (AIP) | |
| 18:45 | Can active plate tectonics leave an observational feature in a planet’s atmosphere? | Lena Noack | Freie Universität Berlin | |
| 19:00 | Stellar space weather effects on habitable-zone planets | Aline Vidotto | Trinity College Dublin & Leiden University | |
| 19:15 | End of Day 3 | |||
Pre-recorded Talks |
| How magnetism of solar-type stars evolve? | Quentin Noraz | Univ. Paris-Saclay | |
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| Dynamically Informed Habitable Zones in Circumbinary Planetary Systems | Nikolaos Georgakarakos | New York University Abu Dhabi | |
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| Panspermia in the context of PLATO’s long-period exo-Earths | Dimitri Veras | University of Warwick | |
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| Model for a rocky planet around the nearest Sun-like stars | Haiyang Wang | Institute for Particle Physics and Astrophysics, ETH Zurich | |
| Thursday 14 October |
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| Time (CEST) | Title | Speaker | Affiliation | |
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Light Curve Analysis (Chair: Sophia Sulis) |
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| 14:00 | PLATO Performance Update (invited) | Juan Cabrera | DLR Berlin | |
| 14:30 | An Overview of Transiting Exoplanet Detection (invited) | Andrew Vanderburg | University of Wisconsin-Madison | |
| 15:00 | Alleviating the Transit Timing Variations bias in transit surveys | Adrien LELEU | Université de Genève | |
| 15:15 | Automated planet validation from transit surveys - lessons from Kepler and potential for PLATO | David Armstrong | University of Warwick | |
| 15:30 | Coffee Break | |||
| 15:45 | SINGLETRANS, the search for single transits of small planets in light curves of space missions | Sascha Grziwa | RIU Planetary Research at the University of Cologne | |
| 16:00 | Poster pitch presentations | |||
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Advances in modelling stellar internal structure and evolution (Chair: Hans-Günter Ludwig) |
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| 16:15 | Stellar modeling in the age of PLATO (invited) | Aldo Serenelli | Institute of Space Sciences - CSIC | |
| 16:45 | Lithium depletion and angular momentum transport in low-mass stars | Thibaut Dumont | University of Geneva | |
| 17:00 | Impact of the transport of chemical elements on the internal structure and surface abundances of stars | Morgan Deal | Instituto de Astrofísica e Ciências do Espaço (IA) | |
| 17:15 | On the Potential of the Reynolds Stress Approach to Model Convective Overshooting in Grids of Stellar Evolution Models | Friedrich Kupka | Univ. of Applied Sciences Technikum Wien | |
| 17:30 | Coffee Break | |||
| 17:45 | Entropy-calibrated models of solar-like stars | Federico Spada | Max Planck Institute for Solar System Resarch | |
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Complementary science topics benefitting from PLATO high-precision photometry (Chair: Konstanze Zwintz ) |
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| 18:00 | The PLATO Complementary Science program (invited) | Andrew Tkachenko | KU Leuven | |
| 18:30 | From TESS to PLATO: A Galactic archaeology perspective | Thibault Boulet | Centro de Astrofísica da Universidade do Porto | |
| 18:45 | Tracers of Exoplanet Composition | Amy Bonsor | Institute of Astronomy, University of Cambridge | |
| 19:00 | Exoplanets in stellar clusters and young associations: the path-way from TESS to PLATO | Domenico Nardiello | Laboratoire d'Astrophysique de Marseille | |
| 19:15 | End of Day 4 | |||
Pre-recorded Talks |
| Analytic Approach for Light Curve Fitting | Yair Judkovsky | Weizmann Institute of Science | |
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| The transport of angular momentum in stellar radiative zones in 2D | Louis Manchon | Max-Planck Institut für Sonnensystemforschung, Göttingen | |
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| The variable sky as seen by TESS: application to PLATO | Mauro Barbieri | Universidad de Atacama | |
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| The temperature, gravity, and frequency scaling relation for delta Scuti stars | Sebastià Barceló Forteza | Universidad de Granada | |
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| Polluted White Dwarfs as Probes of Exoplanetary Interiors | Andrew Buchan | University of Cambridge | |
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| Seismic diagnosis for rapidly rotating g-mode upper-main- sequence pulsators | Hachem Dhouib | Astrophysics Division, CEA Paris-Saclay | |
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| Analysis of eclipsing binaries in multiple stellar systems: the case of V1200 Centauri | Frédéric Marcadon | Nicolaus Copernicus Astronomical Center | |
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| On the age determination of the open cluster α Per with asteroseismology | David Pamos Ortega | University of Granada | |
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| “How to be a connoisseur of stellar light curves” or criteria for reliable frequency extraction in pulsating stars observations | Javier Pascual Granado | Institute of Astrophysics of Andalusia - CSIC | |
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| Searching rotational splittings in δ~Scuti stars using pattern finding techniques | Alejandro Ramón-Ballesta | Instituto de Astrofísica de Andalucía - CSIC | |
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| From protostar to pre-main sequence pulsator: PLATO and the quest for the classification of young stars | Thomas Steindl | University of Innsbruck | |
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| Structure and evolution of young stellar objects: the importance of PLATO observations | Konstanze Zwintz | University of Innsbruck, Institute for Astro- and Particle Physics | |
| Friday 15 October |
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| Time (CEST) | Title | Speaker | Affiliation | |
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Ground-based observations for the confirmation and mass determination of planets (Chair: Annelies Mortier) |
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| 14:00 | Ground-based facilities and techniques for characterising Earth analogues (invited) | Andrew Collier-Cameron | University of St. Andrews | |
| 14:30 | Extremely precise HARPS-N solar RV to overcome the challenge of stellar signal | Xavier Dumusque | University of Geneva | |
| 14:45 | Confirming & detecting circumbinary planets using radial-velocities | Amaury Triaud | University of Birmingham | |
| 15:00 | Stellar characterization, activity, and terrestrial planets: Results from five years of CARMENES spectroscopy | Ansgar Reiners | Institut für Astrophysik Göttingen | |
| 15:15 | Stellar Companions: Hiding the Earth-sized Transiting Planets | David Ciardi | NASA Exoplanet Science Institute - Caltech/IPAC | |
| 15:30 | Coffee Break | |||
| 15:45 | Radial velocity follow-up of young transiting planets: promising results from selected case studies | Mario Damasso | INAF-Astrophysical Observatory of Torino | |
| 16:00 | Discussion | |||
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PLATO in the context of Kepler/K2, TESS, CHEOPS, JWST, Roman, ARIEL and large ground-based observatories. (Chair: Jessie Christiansen) |
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| 16:30 | PLATO-Gaia synergy for studying transiting exoplanets | Aviad Panahi | Tel Aviv University | |
| 16:45 | Optimizing Science Return from Plato’s Observations of the Kepler Field | Jack Lissauer | NASA Ames | |
| 17:00 | Detection and Characterization of Exoplanets Using Current and Future US Observatories (Invited) | Scott Gaudi | Ohio State University | |
| 17:30 | Coffee Break | |||
| 17:45 | High-precision photometry of PLATO targets observed by TESS | Marco Montalto | Universitá di Padova | |
| 18:00 | The future of exoplanet characterisation - the European route (invited) | Ignas Snellen | Leiden Observatory | |
| 18:30 | LIFE – characterizing the climates of terrestrial exoplanets in the wake of PLATO | Tim Lichtenberg | University of Oxford | |
| 18:45 | Concluding remarks | |||
| 19:00 | End of Day 5 | |||
Pre-recorded Talks |
| HARPS3 and opportunities for RV follow-up of PLATO targets | Clark Baker | University of Cambridge | |
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| High-precision characterizations of K2 and TESS planet candidates from the KESPRINT consortium: Outlook for PLATO | Hans Deeg | Instituto de Astrofísica de Canarias | |
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| Toward ground-based detection of exoEarths | Dainis Dravins | Lund Observatory | |
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| PLATOSpec, ground based support for PLATO | Eike Wolf Guenther | Thüringer Landessternwarte Tautenburg | |
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| High-resolution reconnaissance imaging for fulfilling the PLATO science objectives | Markus Janson | Stockholm University | |
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| A robust, empirical approach to determine line-by-line convective blueshift strengths from F to M dwarfs | Florian Liebing | Institut für Astrophysik, University Göttingen | |
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| Posters | |||
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1 |
Exploring the variety of small planets using HARPS-N |
Annelies Mortier |
Kavli Institute, Cavendish Lab., Univ. of Cambridge |
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2 |
Hot Jupiters, Cold Kinematics |
Alexander Mustill |
Lund University, Sweden |
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3 |
Photometric magnetic activity and active-region lifetimes of solar-like stars |
Angela Santos |
The University of Warwick |
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4 |
Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422 |
Alexandr Volvach |
Radio Astronomy Laboratory of Crimean Astrophysical Observatory |
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5 |
The key role of the host star rotational history on the evolution of the planetary system: the case of TOI-849 and Kepler-444. |
Camilla Pezzotti |
University of Geneva |
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6 |
Novel gyrochronology tests with wide-separation binaries |
Diego Godoy-Rivera |
Instituto de Astrofisica de Canarias (IAC) |
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7 |
Transit Timing in the Kepler Field with PLATO: The case for 24 cameras on the Kepler Field. |
Daniel Jontof-Hutter |
University of the Pacific |
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8 |
CHOCOLATE: a new Chromatic Line-Profile Tomography technique to retrieve transmission spectroscopy |
Emma Esparza-Borges |
Instituto de Astrofísica de Canarias (IAC) |
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9 |
Tidal dissipation modelling in gaseous giant planets at the time of space missions |
Hachem DHOUIB |
Astrophysics Division, CEA Paris-Saclay |
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10 |
An assessment of potential Plato Observing strategies to maximize science return from the Kepler Field. |
Jason Rowe |
Bishop's University |
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11 |
The detectability of Saturn-like exoplanetary rings by PLATO |
Leigh Smith |
University of Cambridge |
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12 |
Extended-body corrections to the inverse-square law for spherically symmetric sources |
Mradumay Sadh |
Nicolaus Copernicus Astronomical Center, Warsaw |
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13 |
Prospects for PlatoSim, the end-to-end PLATO Simulator, combined with High Performance Computing |
Nicholas Jannsen |
KU Leuven |
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14 |
TOI-2257 b: A highly eccentric long-period sub-Neptune transiting an M dwarf |
Nicole Schanche |
University of Bern |
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15 |
Magneto-chronology of nearby Sun-like stars |
Philippe Gondoin |
(none) |
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16 |
The star-planet interaction by combining asteroseismic and space weather techniques |
Raffaele Reda |
University of Rome Tor Vergata |
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17 |
ROOSTER, a machine learning tool to determine stellar surface rotation periods in Kepler data |
Sylvain Breton |
AIM - CEA de Saclay/Université de Paris |
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18 |
Study of strange exoplanets |
S.Majal Shiny |
Karunya Institute of Technology and Sciences, Coimbatore |
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19 |
Sweet Cat v2: What stellar homogeneous parameters provide to planetary systems studies |
Sergio Sousa |
Instituo de astrofisica e ciência do espaco |
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20 |
How the stellar flicker noise affects the characterization of planetary transits? |
Sophia SULIS |
Univ. Aix Marseille, LAM, |
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21 |
Estimation of hot Jupiter tidal infall rate in the Galaxy |
Yaroslav Lazovik |
Sternberg Astronomical Institute, Lomonosov Moscow State University |
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22 |
SOAP-GPU: Efficient Spectral Modeling of stellar activity using Graphic Processing Units |
Yinan Zhao |
Observatoire de Genève, Univ. de Genève |
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23 |
The envelope of low-mass stars: the impact of coulomb effect on stellar oscillations |
Ana Brito |
Dept. Matemática Instituto Superior de Gestão |
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24 |
Hierarchically modelling many stars |
Alexander Lyttle |
University of Birmingham |
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25 |
Detecting sub-stellar companions using the stellar pulsation timing method |
Felix Mackebrandt |
Max Planck Institute for Solar System Research |
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26 |
Mixed Modes and the Asteroseismic Surface Term |
Joel Ong |
Yale University |
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27 |
Rotation and flares of M dwarfs with habitable zones accessible to TESS |
Mirjam Bogner |
Institut fuer Astronomie und Astrophysik Tuebingen |
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28 |
The SHERLOCK PIPEline |
Martín Dévora Pajares |
Dpto. Física Teórica y del Cosmos. Universidad de Granada. |
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29 |
Earth-like planets orbiting solar-like stars |
Vardan Adibekyan |
Instituo de astrofisica e ciência do espaco |
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30 |
PLATO's capabilities in studying phase curves |
Vikash Singh |
INAF, Osservatorio Astrofisico di Catania |
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31 |
The Pandora SmallSat |
Thomas Barclay |
NASA GSFC / UMBC |
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32 |
Giant white-light flares on fully convective stars occur at high latitudes |
Ekaterina Ilin |
Leibnitz Institute for Astrophysics, Postdam (AIP) |
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33 |
Spatially resolved solar spectroscopy as benchmark |
Monika Ellwarth |
Institut für Astrofisik, Georg-August Universität Gottingen |
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34 |
Stellar Parameters Via Spectrum Synthesis Of APOGEE DR 16 H-band Spectra Of M Dwarf Stars |
Bárbara Rojas-Ayala |
AI-UTA |
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35 |
Hunting for exoplanets in stellar associations using TESS |
Eleni Evangelia Manthopoulou |
University of Padova |
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36 |
CHEOPS, HARPS-N and TESS: a joint effort to characterize the unexpected planetary system around TOI-561 |
Gaia Lacedelli |
University of Padova |
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37 |
Validation of TESS exoplanet candidates orbiting Solar-analog stars |
Giacomo Mantovan |
University of Padova |
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| 38 | The similarity of multi-planet systems | Jon Fernandez Otegi | Universities of Geneva & Zurich | |
| 39 | Unraveling Solar analogs from PLATO mission: Rotation and activity recovery from simulated light curves | Leandro de Almeida | Laboratóio Nacional de Astrofísica | |
| 40 | NIRPS: the Near-InfraRed Planet Searcher joining HARPS on the 3.6-m | Nolan Grieves | University of Geneva | |
| 41 | Structure of the tidally heated hot Jupiter KELT-9b | Nadine Nettelmann | DLR Berlin | |
| 42 | A fast folding algorithm to produce BLS periodograms in search for transiting planets | Sahar Shahaf | Dept. Particle Physics & Astrophysics, Weizman Institute of Science, Israel | |
| 43 | Characterizing warm Jupiters from TESS single transit events | Solène Ulmer-Moll | Geneva Observatory |
