Splinter Meeting Exoplanets
Exoplanets
Time: Wednesday September 20, 14:00-16:30 and 17:00-19:00
Room: HS1
Organizers: Sandra Jeffers (Göttingen), Alexander Krivov (Jena), Heike Rauer (Berlin), Ansgar Reiners (Göttingen)
Exoplanet discovery and characterization are among the main science drivers in astrophysics. New instruments and mission like CARMENES, CRIRES+, TESS, CHEOPS, and PLATO guarantee tremendous amounts of fresh data for the years to come, and theory is making fast progress explaining the existence and formation and evolution of planets. At the same time, several coordinated programs in the field of exoplanets and the formation of planetary systems are successfully developing in Germany. We want to bring together the exoplanet community and introduce coordinated efforts, and existing and upcoming programs for the next years.
Program
| 14:00 | Sandra Jeffers: |
| Welcome and introduction |
| 14:05 | Heike Rauer: |
| SPP1992: Exploring the Diversity of Extrasolar Planets |
| 14:40 | Ansgar Reiners: |
| Blue Planets around Red Stars - DFG Research Unit about the CARMENES Search for Exoplanets |
| 15:00 | Trifon Trifonov: |
| First results from CARMENES visual-channel radial-velocity measurements |
| 15:20 | Alexis Smith: |
| An Earth-sized planet transiting an M-dwarf in a 4.3-hour orbit |
| 15:40 | Matthias Mallonn: |
| The optical slope in exoplanet spectra and a host star variability survey |
| 16:00 | Mahmoudreza Oshagh: |
| Detecting the variation of measured spin-orbit angles of exoplanet due to the stellar activity |
16:30-17:00 Coffee Break & Poster Session (Foyer Physics)
| 17:00 | Ronald Redmer: |
| Matter Under Planetary Interior Conditions |
| 17:20 | Alexander Krivov: |
| Debris Disks in Planetary Systems |
| 17:40 | Vera Wolthoff: |
| Evolution of Planetary Systems on the Giant Branch |
| 18:00 | Sebastian Kohl: |
| A search for bow shocks around hot gaseous planets |
| 18:20 | Mark Booth: |
| ALMA Observations of Planetary Systems |
| 18:40 | Florian Kirchschlager: |
| Constraints on the structure of hot exozodiacal dust belts and their observability in the MIR |