We provide a comprehensive review of major developments in our understanding of gamma-
ray bursts, with particular focus on the discoveries made within the last fifteen years when …

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 …

Abstract Gamma-Ray Bursts (GRBs) are rapid, bright flashes of radiation peaking in the
gamma-ray band occurring at an average rate of one event per day at cosmological …

For decades, gamma-ray bursts (GRBs) have been broadly divided into long-and short-
duration bursts, lasting more or less than 2 s, respectively. However, this dichotomy does not …

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 mechanism responsible for the prompt emission of gamma‐ray bursts (GRBs) is still a
debated issue. The prompt phase‐related GRB correlations can allow discriminating among …

We report the results of our observing campaign on GRB 140903A, a nearby (z= 0.351)
short-duration (T 90∼ 0.3 s) gamma-ray burst discovered by Swift. We monitored the X-ray …

The gamma-ray burst GRB 221009A, known as the" brightest of all time," is the closest
energetic burst detected so far, with an energy of E γ, iso∼ 10 55 erg. This study aims to …

We investigated the rest-frame spectral lags of two complete samples of bright long (50) and
short (6) gamma-ray bursts (GRB) detected by Swift. We analysed the Swift/Burst Alert …

Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a
dedicated mission, launched in December 2020, for gamma-ray transients, including …