activity
19972026
most citedGamma-ray bursts from internal shocks in a relativistic wind: temporal and spectral properties

476 citations · 1.8k across the 39 of their papers we have counts for

collaborators

38 papers

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…

astro-ph.HE2026

XRF 241001A/SN 2024aiiq: A faint soft X-ray transient detected by SVOM with a broad-line type Ic supernova revealed by JWST

B. Schneider, M. Brunet, B. P. Gompertz +61

X-ray flashes (XRFs) are a type of gamma-ray burst (GRB) with prompt emission predominantly below 30 keV and have been poorly detected by previous missions. The advent of the SVOM…

astro-ph.HE2025★ 6 cited

GRB 221009A and the Apparently Most Energetic Gamma-Ray Bursts

J-L. Atteia, L. Bouchet, J-P. Dezalay +7

Gamma-Ray Bursts (GRBs) are often referred to as the most luminous explosions in the Universe, due to their short and highly luminous prompt emission. This apparent luminosity, how…

astro-ph.HE2023★ 1 cited

Ending the prompt phase in photospheric models of gamma-ray bursts

Filip Alamaa, Frédéric Daigne, Robert Mochkovitch

The early steep decay, a rapid decrease in X-ray flux as a function of time following the prompt emission, is a robust feature seen in almost all gamma-ray bursts with early enough…

astro-ph.HE2023★ 11 cited

The Signature of Refreshed Shocks in the of Afterglow of GRB030329

Michael J. Moss, Robert Mochkovitch, Frédéric Daigne +2

GRB030329 displays one clear and, possibly, multiple less intense fast-rising () jumps in its optical afterglow light curve. The decay rate of the optical light cu…

astro-ph.HE2021★ 21 cited

Flares in gamma-ray burst X-ray afterglows as prompt emission from slightly misaligned structured jets

Raphaël Duque, Paz Beniamini, Frédéric Daigne +1

We develop a model to explain the flaring activity in gamma-ray burst X-ray afterglows within the framework of slightly misaligned observers to structured jets. We suggest that fla…