Sunday, 14th September |
18:00 - 20:00 |
Welcome and Registration |
Monday, 15th September |
08:40 - 09:00 |
Registration |
09:00 - 09:30 |
Conference opening With the presence of:
- Professor Pedro Avelino (Director of the Centro de Astrofísica da Universidade do Porto)
- Professor Paulo Garcia (Member of the ESO Council, in representation of the Fundação para a Ciência e Tecnologia)
- Professor Sebastião Feyo de Azevedo (Rector of the University of Porto)
- Professor Nuno Crato (Minister of Education and Science)
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Session I: Latest results from exoplanet research: observations Chairperson: Christophe Lovis |
09:30 - 10:00 |
IT |
Toward Reliable Planet Occurrence Rates With Kepler |
N. Batalha |
10:00 - 10:20 |
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Occurrence Doesn't Just Happen: Revisiting the Frequency of Earth-Size Planets around Kepler Stars |
E. Gaidos |
10:20 - 10:40 |
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Prevalence of Earth-size planets orbiting Sun-like stars |
E. Petigura |
10:40 - 11:10 |
Coffee Break and Poster View |
11:10 - 11:30 |
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The shortest-period planets |
R. Sanchis-Ojeda |
11:30 - 11:50 |
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Two New Kepler Circumbinary Planets |
W. Welsh |
11:50 - 12:10 |
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The Mass-Radius Relation for 65 Exoplanets Smaller than 4 Earth Radii |
L. Weiss |
12:10 - 12:30 |
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Space-based characterization of super-Earth exoplanets |
B.-O. Demory |
12:30 - 14:00 |
Lunch Break |
Session I: Latest results from exoplanet research: observations Chairperson: Guillermo Gonzalez |
14:00 - 14:20 |
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The Prevalence of Small Planets Around Small Stars from Kepler |
C. Dressing |
14:20 - 14:50 |
IT |
From Radial Velocities to a Planetary Census |
S. Udry |
14:50 - 15:10 |
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HARPS-N Contributions to the Mass-Radius Diagram for Rocky Exoplanets |
D. Latham |
15:10 - 15:30 |
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The atmospheres of warm super-Earths: HD 97658b as a case study |
D. Dragomir |
15:30 - 15:50 |
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How Rocky Are They? The Composition Distribution of Kepler's Sub-Neptune Planet Candidates within 0.15 AU |
A. Wolfgang |
15:50 - 16:20 |
Coffee Break and Poster View |
Session II: Future instruments and methodologies for planet detection and characterization Chairperson: Xavier Dumusque |
16:20 - 16:50 |
IT |
The Transiting Exoplanet Survey Satellite |
J. Winn |
16:50 - 17:10 |
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Machine Learning Approaches to Vetting Transiting Planet Signatures in Photometric Light Curves |
J. Jenkins |
17:10 - 17:40 |
IT |
The CHEOPS mission |
D. Ehrenreich |
17:40 - 18:10 |
IT |
PLATO - The habitable zone terrestrial planet explorer |
D. Pollacco |
Tuesday, 16th September |
Session II: Future instruments and methodologies for planet detection and characterization Chairperson: Sérgio Sousa |
09:15 - 09:45 |
IT |
Exoplanets at the E-ELT era |
G. Chauvin |
09:45 - 10:15 |
IT |
Characterizing Earth-like planets using the Extremely Large Telescopes |
I. Snellen |
10:15 - 10:35 |
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The WFIRST-AFTA Exoplanet Microlensing Survey |
D. Bennett |
10:35 - 10:55 |
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Exoplanet characterisation with the JWST/MIRI instrument |
P.-O. Lagage |
10:55 - 11:20 |
Coffee Break and Poster View |
11:20 - 11:50 |
IT |
ESPRESSO and beyond |
F. Pepe |
11:50 - 12:10 |
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CARMENES |
A. Quirrenbach |
12:10 - 12:30 |
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The Search for Planets at Longer Wavelengths: Prospects, Challenges, and Surprises |
A. Reiners |
12:30 - 14:00 |
Lunch Break |
Session III: Astrophysical noise in exoplanet searches Chairperson: Jon Jenkins |
14:00 - 14:30 |
IT |
Stellar activity in transit and RV planet searches: synergies and challenges |
S. Aigrain |
14:30 - 15:00 |
IT |
The Impact of Stellar Variability on Kepler's Search for Transiting Exoplanets |
J. Christiansen |
15:00 - 15:20 |
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Goldilocks Can't Stay Here: Habitable Zone Planets Around Gliese 581 are Stellar Activity Signals |
P. Robertson |
15:20 - 15:40 |
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The interesting case of HD41248: stellar activity, no planets? |
J. Faria |
15:40 - 16:00 |
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Understanding the stellar activity impact on radial velocity measurements |
E. Hébrard |
16:00 - 16:30 |
Coffee Break and Poster View |
16:30 - 17:00 |
IT |
Gliese 667C Signals and Noise |
P. Gregory |
17:00 - 17:30 |
IT |
Astrophysical noises affecting radial velocity planet searches |
X. Dumusque |
17:30 - 17:50 |
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Disentangling Low-mass Planetary Signals and Stellar Surface Magneto-convection |
H. Cegla |
17:50 - 18:10 |
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Effect of stellar activity on the high-precision transmission spectra: Can occultation of a plage mimic the signature of a blue sky? |
M. Oshagh |
18:10 - 18:30 |
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Planets and Stellar Activity: Hide and Seek in the CoRoT-7 system |
R. Haywood |
Wednesday, 17th September |
Session IV: The precise characterization of stars with planets Chairperson: Ansgar Reiners |
9:30 - 10:00 |
IT |
Directly determined physical properties of late-type stars |
T. Boyajian |
10:00 - 10:30 |
IT |
The Small Stars And Their Small Planets |
B. Rojas-Ayala |
10:30 - 10:50 |
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Metallicity determination for M dwarfs from high-resolution IR spectra |
S. Lindgren |
10:50 - 11:20 |
Coffee Break and Poster View |
11:20- 11:50 |
IT |
Stellar Parameter Determination |
B. Smalley |
11:50 - 12:10 |
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Deriving accurate logg values for planet host stars |
A. Mortier |
12:10 - 12:30 |
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Using simultaneous visible and infrared observations to better constrain stellar activity |
C. Danielsky |
12:30 - 12:50 |
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Li overabundance in giants. Evidence of planet engulfment? |
M. Adamow |
12:50 |
Lunch Break |
18:00 |
Departure for dinner |
Thursday, 18th September |
Session IV: The precise characterization of stars with planets Chairperson: Elisa Delgado-Mena |
09:30 - 10:00 |
IT |
Detailed characterization of stars with planets |
H. Kjeldsen |
10:00 - 10:20 |
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What asteroseismology can do for exoplanets: validation, eccentricity and obliquity of the bright multiple system Kepler-410 |
V. Van Eylen |
10:20 - 10:40 |
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An ancient extrasolar system with five sub-Earth-size planets |
T. Campante |
10:40 - 11:10 |
Coffee Break and Poster View |
Session V: The star-planet connection: system formation, evolution, and its observational signatures Chairperson: Nuno Santos |
11:10 - 11:40 |
IT |
Star-planet connection: the role of stellar metallicity |
V. Adibekyan |
11:40 - 12:10 |
IT |
The role of metallicity in establishing giant planet dynamics |
R. Dawson |
12:10 - 12:30 |
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The metallicity-planet relation of M dwarfs |
V. Neves |
12:30 - 14:00 |
Lunch Break |
14:00 - 14:20 |
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Three distinct exoplanet regimes inferred from host star metallicities |
L. Buchhave |
14:20 - 14:40 |
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Lithium depletion of planetary-host stars: a new and revealing homogeneous study |
P. Figueira |
14:40 - 15:00 |
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Abundance Anomalies in the Composition of Host Stars |
N. Hinkel |
15:00 - 15:30 |
IT |
Models of Planet Formation |
C. Mordasini/P. Moliere |
15:30 - 15:50 |
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Constraining giant exoplanet composition via host star abundances of planet-building elements |
J. Teske |
15:50 - 16:30 |
Coffee Break and Poster View |
16:30 - 16:50 |
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Planet Traps and Super-Earths: Origins of the Planet-Metallicity Relation and Implications for the Mass-Radius Diagram |
Y. Hasegawa |
16:50 - 17:10 |
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Have planets more time to grow than we thought? |
S. Pfalzner |
17:10 - 17:30 |
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Formation and Dynamical Evolution of Circumbinary Planets: Reconciling Theory with Observation |
N. Haghighipour |
17:30 - 17:50 |
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First ever Gravitational Instability population synthesis models for planet formation |
S. Nayakshin |
21:00 |
Public session/debate |
Friday, 19th September |
Session VI: Star-planet interactions Chairperson: Pedro Figueira |
9:30 - 09:50 |
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Detecting Exoplanetary Magnetic Fields |
J. Llama |
09:50 - 10:10 |
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The effects of stellar winds on the magnetospheres and potential habitability of exoplanets |
V. See |
10:10 - 10:30 |
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An X-ray survey of Hot Jupiter Hosts |
S. Wolk |
10:30 - 11:00 |
IT |
Star-planet magnetic interactions |
A. F. Lanza |
11:00 - 11:40 |
Coffee Break and Poster View |
11:40 - 12:00 |
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Planet-host stars: a magnetic study |
R. Fares |
12:00 - 12:30 |
IT |
The importance of being close to your parent star |
R. Mardling |
12:30 - 12:50 |
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Investigating the Role of Stellar Tides in Hot Jupiters' origin and fate |
F. Valsecchi |