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

Swift has now completed 18 years of mission, during which it discovered thousands of
gamma-ray bursts as well as new classes of high-energy transient phenomena. Its first …

We present the most extensive sample of 45 type I (short) and 275 type II (long) gamma-ray
bursts (GRBs) with known redshift to investigate the correlation between the rest-frame peak …

ABSTRACT A significant fraction (30 per cent) of well-localized short gamma-ray bursts
(sGRBs) lack a coincident host galaxy. This leads to two main scenarios:(i) that the …

We report the results of optical follow-up observations of 29 gravitational-wave (GW) triggers
during the first half of the LIGO–Virgo Collaboration (LVC) O3 run with the Gravitational …

On August 17, 2017, less than two years after the direct detection of gravitational radiation
from the merger of two∼ 30 M⊙ black holes, a binary neutron star merger was identified as …

ABSTRACT GRB 160821B is a short duration gamma-ray burst (GRB) detected and
localized by the Neil Gehrels Swift Observatory in the outskirts of a spiral galaxy at z …

In this paper, we investigate the properties of binary neutron stars (BNSs) and their mergers
by combining population synthesis models for binary stellar evolution (BSE) with …

The discovery of GW170817 and GRB 170817A in tandem with AT 2017gfo cemented the
connection between neutron star mergers, short gamma-ray bursts (GRBs), and kilonovae …