Gamma-ray bursts (GRBs) are divided into two populations,; long GRBs that derive from the
core collapse of massive stars (for example, ref.) and short GRBs that form in the merger of …

We present a comprehensive optical and near-infrared census of the fields of 90 short
gamma-ray bursts (GRBs) discovered in 2005–2021, constituting all short GRBs for which …

We present preexplosion optical and infrared (IR) imaging at the site of the type II supernova
(SN II) 2023ixf in Messier 101 at 6.9 Mpc. We astrometrically registered a ground-based …

We present the stellar population properties of 69 short gamma-ray burst (GRB) host
galaxies, representing the largest uniformly modeled sample to date. Using the Prospector …

We present optical, ultraviolet, and infrared data of the type II supernova (SN II) 2020jfo at
14.5 Mpc. This wealth of multiwavelength data allows us to compare different metrics …

The merger rate density evolution of binary compact objects and the properties of their host
galaxies carry crucial information to understand the sources of gravitational waves. Here, we …

We present a population of 11 of the faintest (> 25.5 AB mag) short gamma-ray burst (GRB)
host galaxies. We model their sparse available observations using the stellar population …

We address the problem of optimally identifying all kilonovae detected via gravitational-
wave emission in the upcoming LIGO/Virgo/KAGRA observing run, O4, which is expected to …

Aims. The locations of binary neutron star (BNS) mergers within their host galaxies encode
the systemic kicks that these systems received in the supernova aftermath. We investigate …

The exact nature of the luminous fast blue optical transient AT 2018cow is still debated. In
this first of a two-paper series, we present a detailed analysis of three Hubble Space …