We report our identification of the optical afterglow and host galaxy of the short-duration
gamma-ray burst sGRB 160821B. The spectroscopic redshift of the host is z= 0.162, making …

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 …

Cosmological probes at any redshift are necessary to reconstruct consistently the cosmic
history. Studying properly the tension on the Hubble constant, H 0, obtained by supernovae …

The gamma-ray burst GRB 211211A and its associated kilonova-like emission were
reported recently. A significant difference between this association event and GRB …

Rapidly spinning, strongly magnetized protoneutron stars (" millisecond protomagnetars")
are candidate central engines of long-duration gamma-ray bursts (GRBs), superluminous …

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 …

Originating from neutron star–neutron star or neutron star–black hole mergers, short gamma-
ray bursts (SGRBs) are the first electromagnetic emitters associated with gravitational waves …

We present the results of a detailed investigation of the prompt and afterglow emission in the
High Energy Stereoscopic System (HESS)-detected GRB 190829A. Swift and Fermi …

We study the long-term () evolution of the accretion disc after a neutron star (NS)–NS or NS–
black hole merger, taking into account the radioactive heating by r-process nuclei formed in …

ABSTRACT A long-lived magnetar, potentially originating from a binary neutron star system,
has been proposed to explain the extended emission observed in certain short-duration …