… 2017a) was a watershed event in astrophysics, marking the first multimessenger detection
of a binary neutron star (BNS) merger. Here, we review the observations of this event and …

… , no detection has been confirmed so far. As for binary neutron star systems, BHNS binaries
allow us to explore a wide range of physical processes, including the neutron star equation …

… the details of the source detection and photometry, including … (2016, Paper I) provide an
overview of the Pan-STARRS … the number of stars per square degree at the 5σ detection limit in …

… properties at the end of the star formation process. We then proceed with an overview of
theoretical models describing the origin and early evolution of multiple star systems in §3. Using …

… We all agree what a star cluster is when we see one, but coming up with a quantitative … a
star cluster is a group of stars, but so are galaxies, so not all stellar groupings are star clusters. …

… The detector is read out using a detector controller system supplied by Astronomical … In
order to select a pure sample of stars (ie, point sources), we require that all astrometric calibrators …

… Neutron star mergers are the canonical multimessenger events: they have been observed
… , the expected observational signatures, and estimated detection rates for the next decade. I …

… detection and its profound impact on the entire computer vision field. If we consider today’s
object detection … in history, detection datasets, metrics, fundamental building blocks of the …

… Here, we provide an overview of the impact of spatially resolved infrared, … , star formation
and active galactic nuclei as well as their interplay in local LIRGs. We also present an overview …

… and GW170817, as well as on the new questions raised by the first detection. For a more
general overview of NS mergers, we refer readers to Reference 22. For more detailed …