S. Antier

Observation of Gravitational Waves from the Coalescence of a $2.5\text{-}4.5~M_\odot$ Compact Object and a Neutron Star

A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Predicting electromagnetic counterparts using low-latency gravitational-wave data products

Implications of the search for optical counterparts during the first six months of the Advanced LIGO’s and Advanced Virgo’s third observing run: possible limits on the ejecta mass and binary properties