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 …

The binary neutron star (BNS) merger GW170817 was the first astrophysical source
detected in gravitational waves and multiwavelength electromagnetic radiation. The almost …

The detection of GW170817, it's extensive multi-wavelength follow-up campaign, and the
large amount of theoretical development and interpretation that followed, have resulted in a …

The detections of GW170817 and GRB 170817A revealed that at least some short gamma-
ray bursts (sGRB) are associated with the merger of neutron-star compact binaries. The …

The milestone of GW 170817-GRB 170817A-AT 2017gfo has shown that gravitational wave
(GW) is produced during the merger of neutron star-neutron star/black hole and that in …

In the faint short gamma-ray burst sGRB 170817A followed by the gravitational waves (GWs)
from a merger of two neutron stars (NSs) GW170817, the spectral peak energy is too high to …

The paper 'The Ep, i–Eiso correlation: type I gamma-ray bursts and the new classification
method'was published in MNRAS, 492, 1919–1936 (2020). After publication of the paper, a …

In this paper we carry out a semi-analytic general relativistic study of a Gamma-Ray Bursts
(GRB) jet that is breaking out of a cocoon or stellar envelope. We solve hydrodynamic …

The prompt emission of gamma-ray bursts (GRBs) is a long-standing problem. The spectral-
lag phenomenon can provide us with some clues about the emission mechanism. By …

Aims. There exists inevitable scatter in the intrinsic luminosity of gamma-ray bursts (GRBs). If
there is relativistic beaming in the source, viewing angle variation necessarily introduces …