Constraining possible $\gamma$-ray burst emission from GW230529 using
Swift-BAT and Fermi-GBM
Constraining possible $\gamma$-ray burst emission from GW230529 using
Swift-BAT and Fermi-GBM
GW230529 is the first compact binary coalescence detected by the LIGO-Virgo-KAGRA collaboration with at least one component mass confidently in the lower mass-gap, corresponding to the range 3-5$M_{\odot}$. If interpreted as a neutron star-black hole merger, this event has the most symmetric mass ratio detected so far and therefore has …