Splinter Meetings
Splinter meetings will be held in parallel and may optionally last one or two afternoon sessions during the conference.
Below you can find the list of the splinter meetings accepted by the SOC, including links to their websites.
Please note: Abstract submission for all splinters is done centrally through the Abstract Submission on this Website. Please do not send your abstracts directly to the convenors of the splinter meetings!
| Splinter | Title | Days | Room | ||
|---|---|---|---|---|---|
| Tue | Wed | Thu | |||
| Activity | Solar and stellar activity and variability | X | Auditorium MPS | ||
| AGN | Active Galactic Nuclei | X | HS4 | ||
| CCAT | CCAT-prime: new submillimeter science opportunities | X | Auditorium MPS | ||
| Computation | Computational Astrophysics | X | X | HS3 | |
| E-Science | E-Science, E-Infrastructures, and Virtual Observatory (Machines of Discovery) | X | X | SR17 | |
| Education | Astronomy and Education | X | HS5 | ||
| eROSITA | eROSITA is Coming! Opportunities to Study Cosmology and Large Scale Structure with X-ray Selected Clusters and AGN | X | HS4 | ||
| Euclid | The Euclid space mission | X | HS2 | ||
| Exoplanets | Exoplanets | X | HS1 | ||
| HiRes | High-Resolution Solar Imaging, Spectroscopy, and Polarimetry - Recent Developments in Science and Instrumentation | X | Auditorium MPS | ||
| HotStars | Hot Stars and Binary Evolution | X | HS3 | ||
| Non-Thermal | Surveying the non-thermal Universe | X | HS4 | ||
| Plasma | Space Plasma Processes in Stellar and Planetary Environments | X | D+E+F MPS | ||
| Populations | Stellar Populations in and around the Milky Way | X | X | HS5 | |