WG 3 Leader: Dr. Sebastiano Bernuzzi 

Task Leader: Dr. Alessandro Patruno 

Task Leader: Dr. Morgane Fortin 


PHAROS will aim at answering which different gravitational signals are expected from different neutron star systems, and how can they be characterized with real observables, and distinguished from other gravitational wave emitters.



• Determine micro-physical and observational inputs required for models.

• Determine standards to allow gravitational wave observers to use models effectively.

• Closer collaboration between theorists and observers to develop models.


Participants: TBD