Gamma-ray burst (GRB) afterglow emission can be observed from sub-TeV to radio
wavelengths, though only 6.6% of observed GRBs present radio afterglows. We examine …

Gamma-ray Bursts (GRBs) are highly energetic events that can be observed at extremely
high redshift. However, inherent bias in GRB data due to selection effects and redshift …

Gamma-ray bursts (GRBs) are very energetic cosmological transients. Long GRBs are
usually associated with Type Ib/c supernovae (SNe), and we refer to them as GRB-SNe …

The immense power of gamma-ray bursts (GRBs) makes them ideal probes of the early
universe. By using absorption lines in the afterglows of high-redshift GRBs, astronomers can …

We report the results of an extensive set of simulations exploring the sensitivity of the
BlackCAT CubeSat to long-duration gamma-ray bursts (GRBs). BlackCAT is a NASA APRA …

We analyse two distinct samples of gamma-ray bursts (GRBs), with and without radio
afterglow emission. We use an updated sample of 211 GRBs and find, in agreement with …

We explore the possibility that radio-loud gamma-ray bursts (GRBs) result from the collapse
of massive stars in interacting binary systems, while radio-quiet GRBs are produced by the …

Aims. Long gamma-ray bursts (LGRBs) have been shown to be powerful probes of the
Universe, in particular for studying the star formation rate up to very high redshift (z∼ 9) …

Neutron star mergers are astrophysicalgold mines,'synthesizing over half of the elements
heavier than iron through rapid neutron capture nucleosynthesis. The observation of the …

Some short gamma-ray bursts (SGRBs) exhibit a short-duration and spectral hard emission
(referred to as a “hard spike”) followed by a slightly longer soft emission (known as a “soft …