The symposium will be organized around a morning plenary session and two parallel sessions in the afternoon.
- 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.
Plenary Sessions (9:00 am - 12:35 pm)
(June 22) MGW1 – NS Population and Environment
A time slot of 30 minutes is allocated to short 1-slide presentations advertising the content of the displayed posters.
(June 23) MGW2 – NSs and Magnetars as Sources of Gravitational Waves
(June 24) MGW3 – NS and Magnetar Emission Processes
(June 26) MGW5 – NS Astrophysics with Future Observatories