collaborators

17 papers

astro-ph.HE2026

Exploring cosmic magnetism with gamma-ray burst afterglow emission

Paolo Da Vela, Davide Miceli, Lara Nava +1

The paper investigates whether delayed gamma‑ray emission (pair‑echo) from TeV afterglows of gamma‑ray bursts can be detected with CTAO to constrain intergalactic magnetic field st…

astro-ph.HE2026

Late-time X-ray afterglows of GRBs: Implications for particle acceleration at relativistic shocks

Zhi-Qiu Huang, Om Sharan Salafia, Lara Nava +2

Particle-in-cell (PIC) numerical simulations are currently among the most advanced tools to investigate particle acceleration at relativistic shocks. Still, they come with limitati…

astro-ph.HE2026

Colour evolution in the radio afterglow of GRB 241025A

S. Giarratana, O. S. Salafia, L. Nava +10

We present the observing campaign of the afterglow of GRB241025A, a gamma-ray burst (GRB) whose prompt emission has been simultaneously detected by Swift, Einstein Probe, Fermi/GBM…

astro-ph.HE2026

Gamma-ray Bursts in the Radio Sky: the Role of the SKA-VLBI

Stefano Giarratana, Om Sharan Salafia, Xue-Feng Wu +6

Radio observations of -ray bursts (GRBs) employing the very long baseline interferometry (VLBI) technique provide us with fundamental information on the dynamics and the geomet…

astro-ph.HE2026

A self-consistent explanation of the MeV line in GRB 221009A unveils a dense circum-stellar medium

O. S. Salafia, A. Celotti, E. Sobacchi +6

GRB~221009A has been the brightest gamma-ray burst (GRB) observed to date, and its afterglow has been characterized with unprecedented detail at TeV energies by LHAASO. Quite puzzl…

astro-ph.HE2026

Time lags as proxy of spectral evolution in gamma-ray bursts

C. Maraventano, F. Daigne, R. Mochkovitch +3

Positive lags in gamma-ray bursts (GRBs), where hard photons anticipate softer ones, provide a unique window into the temporal evolution of their prompt emission. Negative lags, wh…