The symposium will be organized around a plenary session (9:00-12:35 am CET) and two parallel sessions (2:30 am – 6:00 pm CET). All the talks will be living. In order to enlarge the access to the talks for registered people living in different time zones, all the living talk will be recordered, and the records made accessible to the symposium particpants.
- Plenary sessions are designed to give a broad and interdisciplinary overview of neutron stars, their gravitational wave and electromagnetic emission. They will summarize the current status of the art and highlight the most recent progresses in the field of neutrons star astrophysics, of magnetars, gravitational wave sources and their electromagnetic counterparts.
- The parallel sessions will instead provide a deeper insight into specific questions on the physics of the magnetar on one side, and neutron stars as sources of gravitational waves, kilonovae and gamma ray burst on the other.
A time slot of 30 minutes is allocated to short 1-slide presentations advertising the content of the displayed posters.