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20172024
most citedEarly X-ray Flares in GRBs

54 citations · 346 across the 17 of their papers we have counts for

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14 papers · 1 filter

astro-ph.HE2024

Temporal and Spectral Analysis of the Unique and Second Brightest Gamma-Ray Burst GRB 230307A: Insights from GECAM and Fermi/GBM Observations

R. Moradi, C. W. Wang, B. Zhang +6

In this study, we present the pulse profile of the unique and the second brightest gamma-ray burst GRB 230307A, and analyze its temporal behavior using a joint GECAM--Fermi/GBM tim…

astro-ph.HE2021★ 24 cited

The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs

R. Ruffini, R. Moradi, J. A. Rueda +14

We recall evidence that long gamma-ray bursts (GRBs) have binary progenitors and give new examples. Binary-driven hypernovae (BdHNe) consist of a carbon-oxygen core (CO$_{\rm core}…

astro-ph.HE2021★ 5 cited

Timing techniques applied to distributed modular high-energy astronomy: the HERMES project

A. Sanna, A. F. Gambino, L. Burderi +15

The HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites -- Technologic and Scientific Pathfinder) is an in-orbit demonstration of the so-called distributed astronomy con…

astro-ph.HE2021★ 24 cited

The HERMES-Technologic and Scientific Pathfinder

F. Fiore, L. Burderi, M. Lavagna +12

HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites Technologic and Scientific Pathfinder) is a constellation of six 3U nano-satellites hosting simple but innovative X-r…

astro-ph.HE2019★ 33 cited

Magnetic Fields and Afterglows of BdHNe: Inferences from GRB 130427A, GRB 160509A, GRB 160625B, GRB 180728A and GRB 190114C

Jorge A. Rueda, R. Ruffini, M. Karlica +2

GRB 190114C is the first binary-driven hypernova (BdHN) fully observed from the initial supernova appearance to the final emergence of the optical SN signal. It offers an unprecede…

astro-ph.HE2019★ 6 cited

Self-similarity and power-laws in GRB 190114C

R. Ruffini, Liang Li, R. Moradi +10

Following Fermi and NOT observations, Ruffini et al. (2019b) soon identified GRB 190114C as BdHN I at z=0.424, it has been observed since, with unprecedented accuracy, [...] all th…