activity
20182026
most citedTwo Predictions of supernova: GRB 130427A / SN 2013cq and GRB 180728A / SN 2018fip

36 citations · 60 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2026

GRB 220101A: a most energetic erg long GRB triggered by two supernovae 3.5 seconds apart

R. Ruffini, Y. Aimuratov, L. M. Becerra +10

GRB 220101A is a long GRB, with a total energy exceeding erg with a redshift and one of the largest ever high-quality multi-wavelength observational coverage,…

astro-ph.HE2024★ 2 cited

Ten Supernova-rise in Binary Driven Gamma-ray Bursts

R. Ruffini, C. L. Bianco, Liang Li +6

The observation of a gamma-ray burst (GRB) associated with a supernova (SN) coincides remarkably with the energy output from a binary system comprising a very massive carbon-oxygen…

astro-ph.HE2023★ 4 cited

Probing electromagnetic-gravitational wave emission coincidence in type I binary-driven hypernova family of long GRBs at very-high redshift

C. L. Bianco, M. T. Mirtorabi, R. Moradi +7

The repointing time of the XRT instrument on the Neil Gehrels Swift Observatory satellite has posed challenges in observing and studying the early X-ray emissions within $\approx40…

astro-ph.HE2023★ 18 cited

GRB-SN Association within the Binary-Driven Hypernova Model

Y. Aimuratov, L. M. Becerra, C. L. Bianco +11

The observations of supernovae (SNe) Ic occurring after the prompt emission of long gamma-ray bursts (GRBs) are addressed within the binary-driven hypernova (BdHN) model where GRBs…

astro-ph.HE2018★ 36 cited

Two Predictions of supernova: GRB 130427A / SN 2013cq and GRB 180728A / SN 2018fip

Yu Wang, Jorge A. Rueda, Remo Ruffini +4

On 2018 July 28, GRB 180728A triggered \textit{Swift} satellites and, soon after the determination of the redshift, we identified this source as a type II binary-driven hypernova (…