… On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by the …

… On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by the …

… multi-messenger BNS merger constraints described in this work can be combined using
the statistical framework described by Miller et al. (2019), providing more stringent constraints …

… The GW170817 event has constrained neutron star properties [6], [15], [13], [16], [20], [19] …
electromagnetic observations [9]. This review summarizes the multi-messenger observations of …

… to classify observed EM transients such as GRB200826A 36 , and to combine information from
multi-messenger observations … on the multi-messenger nature of compact-binary mergers. …

… We present realistic expectations for the number and properties of neutron star binary mergers
to be detected as multi-messenger sources during the upcoming fourth observing run (O4…

On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the …

On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the …

… the binary neutron star merger GW170817, and subsequently by astronomers of transient
counterparts across the electromagnetic spectrum, has initiated the era of “multi-messenger …

… and provide insights into the population of merging binaries. This doctoral thesis aims to
leverage multi-messenger observations of binary neutron star mergers in two ways. I developed …