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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.
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 25) MGW4 – NS and Gamma-ray Burst Connectionv
(June 26) MGW5 – NS Astrophysics with Future Observatories

June 22nd, Mon

  • MWG1 - Invited

    -

    NS Population and Environment

  • MWG1 - Invited

    -

    NS Population and Environment

  • Coffee Break

    -

  • MWG1 - Invited

    -

    NS Population and Environment

  • MWG1 - Contributed

    -

    NS Population and Environment

  • MWG1 - Poster

    -

    NS Population and Environment

    Poster Session

June 23rd, Tue

  • MWG2 - Invited

    -

    NSs and Magnetars as Sources of Gravitational Waves

  • MWG2 - Invited

    -

    NSs and Magnetars as Sources of Gravitational Waves

  • Coffee Break

    -

  • MWG2 - Invited

    -

    NSs and Magnetars as Sources of Gravitational Waves

  • MWG2 - Contributed

    -

    NSs and Magnetars as Sources of Gravitational Waves

  • MWG2 - Contributed

    -

    NSs and Magnetars as Sources of Gravitational Waves

June 24th, Wed

  • MWG3 - Invited

    -

    NS and Magnetar Emission Processes

  • MWG3 - Invited

    -

    NS and Magnetar Emission Processes

  • Coffee Break

    -

  • MWG3 - Invited

    -

    NS and Magnetar Emission Processes

  • MWG3 - Contributed

    -

    NS and Magnetar Emission Processes

  • MWG3 - Contributed

    -

    NS and Magnetar Emission Processes

June 25th, Thu

  • MWG4 - Invited

    -

    NS and Gamma-ray Burst Connection

  • MWG4 - Invited

    -

    NS and Gamma-ray Burst Connection

  • Coffee Break

    -

  • MWG4 - Invited

    -

    NS and Gamma-ray Burst Connection

  • MWG4 - Contributed

    -

    NS and Gamma-ray Burst Connection

  • MWG4 - Contributed

    -

    NS and Gamma-ray Burst Connection

June 26th, Fri

  • MWG5 - Invited

    -

    NS Astrophysics with Future Observatories

  • MWG5 - Invited

    -

    NS Astrophysics with Future Observatories

  • Coffee Break

    -

  • MWG5 - Invited

    -

    NS Astrophysics with Future Observatories

  • MWG5 - Contributed

    -

    NS Astrophysics with Future Observatories

  • MWG5 - Contributed

    -

    NS Astrophysics with Future Observatories

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