activity
20162024
most citedA very-high-energy component deep in the Gamma-ray Burst afterglow

274 citations · 2.1k across the 43 of their papers we have counts for

collaborators

43 papers

astro-ph.HE2024

The Galactic population of canonical pulsars II

Mattéo Sautron, Jérôme Pétri, Dipanjan Mitra +1

Pulsars are highly magnetized rotating neutron stars, emitting in a broad electromagnetic energy range. Reproducing the observed pulsars population refines our understanding of the…

astro-ph.HE2022

The Galactic population of canonical pulsars

Ludmilla Dirson, Jérôme Pétri, Dipanjan Mitra

Current wisdom accounts to the diversity of neutron star observational manifestations to their birth scenarios, influencing their thermal and magnetic field evolution. Among the ki…

astro-ph.HE2022★ 16 cited

Phenomenological modelling of the Crab Nebula's broad band energy spectrum and its apparent extension

Ludmilla Dirson, Dieter Horns

The Crab Nebula emits bright non-thermal radiation from radio to the most energetic photons. The underlying physical model of a relativistic wind from the pulsar terminating in a h…

astro-ph.HE2021★ 13 cited

Searching for TeV gamma-ray emission from SGR\,1935+2154 during its 2020 X-ray and radio bursting phase

H. E. S. S. Collaboration, :, H. Abdalla +251

Magnetar hyperflares are the most plausible explanation for fast radio bursts (FRB) -- enigmatic powerful radio pulses with durations of several milliseconds and high brightness te…

astro-ph.HE2021

Evidence of 100 TeV -ray emission from HESS J1702-420: A new PeVatron candidate

L. Giunti, B. Khelifi, K. Kosack +1

The identification of active PeVatrons, hadronic particle accelerators reaching the knee of the cosmic-ray spectrum (at the energy of few PeV), is crucial to understand the origin…

astro-ph.HE2021★ 13 cited

LMC N132D: A mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV

H. E. S. S. Collaboration, :, H. Abdalla +233

We analyzed 252 hours of High Energy Stereoscopic System (H.E.S.S.) observations towards the supernova remnant (SNR) LMC N132D that were accumulated between December 2004 and March…