most citedTeraelectronvolt emission from the -ray burst GRB 190114C

286 citations · 557 across the 6 of their papers we have counts for

collaborators

14 papers

astro-ph.HE20209 cited

Studying the nature of the unidentified gamma-ray source HESS J1841-055 with the MAGIC telescopes

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +184

We investigate the physical nature and origin of the gamma-ray emission from the extended source HESS J1841-055 observed at TeV and GeV energies. We observed HESS J1841-055 at TeV…

astro-ph.HE2020226 cited

Observation of inverse Compton emission from a long -ray burst

V. A. Acciari, S. Ansoldi, L. A. Antonelli +301

Long-duration gamma-ray bursts (GRBs) originate from ultra-relativistic jets launched from the collapsing cores of dying massive stars. They are characterised by an initial phase o…

astro-ph.HE2020286 cited

Teraelectronvolt emission from the -ray burst GRB 190114C

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +177

Gamma-ray bursts (GRBs) of the long-duration class are the most luminous sources of electromagnetic radiation known in the Universe. They are generated by outflows of plasma ejecte…

astro-ph.HE202033 cited

Testing two-component models on very-high-energy gamma-ray emitting BL Lac objects

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +201

Context. It has become evident that one-zone synchrotron self-Compton models are not always adequate for very-high-energy (VHE) gamma-ray emitting blazars. While two-component mode…

astro-ph.HE2020

A search for dark matter in Triangulum II with the MAGIC telescopes

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +172

We present the first results from very-high-energy observations of the dwarf spheroidal satellite candidate Triangulum II with the MAGIC telescopes from 62.4 hours of good-quality…

astro-ph.HE2020

MAGIC very large zenith angle observations of the Crab Nebula up to 100 TeV

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +169

Aims: We aim to measure the Crab Nebula gamma-ray spectral energy distribution in the ~100 TeV energy domain and test the validity of existing leptonic emission models at these hig…