Short gamma-ray bursts (SGRBs) are now known to be the product of the merger of two
compact objects. However, two possible formation channels exist: neutron star–neutron star …

We examine the relationship between a number of long gamma-ray burst (lGRB) properties
(isotropic emitted energy, luminosity, intrinsic duration, jet opening angle) and redshift. We …

In order to obtain an overview of gamma-ray bursts (GRBs), we need a full sample. In this
paper, we collected 6289 GRBs (from GRB 910421 to GRB 160509A) from the literature …

Distinct X-ray plateau and flare phases have been observed in the afterglows of gamma-ray
bursts (GRBs), and most of them should be related to central engine activities. In this paper …

It is generally supposed that a transition from the normal decay phase (decay slope∼− 1) to
a steeper phase (decay slope∼− 2) could be suggested as a jet break. The jet opening …

The empirical classification of gamma-ray bursts (GRBs) into long and short GRBs based on
their durations is already firmly established. This empirical classification is generally linked …

We present and perform a detailed analysis of multiwavelength observations of GRB
140102A, an optical bright GRB with an observed reverse shock (RS) signature …

Context. X-ray absorbing column densities (NH) are used as a parameter to quantify the
amount of absorbing material along the line of sight. The high values found for long gamma …

The discovery of cosmic neutrino flux by IceCube, and the multi-messenger observations of
gravitational event GW170817 ushered in the era of multi-messenger astronomy. Since the …