activity
20142025
most citedGamma-ray blazar spectra with H.E.S.S. II mono analysis: the case of PKS 2155-304 and PG 1553+113

38 citations · 90 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2025★ 4 cited

Detection of molecular clouds in the PeVatron candidate source LHAASO J03415258 by the Nobeyama 45-m radio telescope

Naomi Tsuji, Shunya Takekawa, Kaya Mori +8

We report a new CO observation survey of LHAASO J03415258 using the Nobeyama Radio Observatory (NRO) 45-m telescope. LHAASO J03415258 is one of the unidentified ultra-high-en…

astro-ph.HE2025★ 7 cited

eROSITA X-ray Analysis of the PeVatron Candidate Westerlund 1

Konstantin Haubner, Manami Sasaki, Alison Mitchell +7

It is unclear which fraction of cosmic rays above an energy of 1 PeV is accelerated by the observed Galactic PeVatron population. These sources' gamma-ray data is typically degener…

astro-ph.HE2021★ 2 cited

The young massive stellar cluster Westerlund 1 in rays as seen with H.E.S.S

Lars Mohrmann, Andreas Specovius, Romed Rauth +2

Massive stellar clusters have recently been hypothesised as candidates for the acceleration of hadronic cosmic rays up to PeV energies. Previously, the H.E.S.S. Collaboration has r…

astro-ph.HE2021★ 3 cited

Detection of new Extreme BL Lac objects with H.E.S.S. and Swift XRT

Mathieu de Bony de Lavergne, Tomas Bylund, Manuel Meyer +2

Extreme high synchrotron peaked blazars (EHBLs) are amongst the most powerful accelerators found in nature. Usually the synchrotron peak frequency of an EHBL is above Hz…

astro-ph.IM2021

Astronomy outreach in Namibia: H.E.S.S. and beyond

Hannah Dalgleish, Heike Prokoph, Sylvia Zhu +6

Astronomy plays a major role in the scientific landscape of Namibia. Because of its excellent sky conditions, Namibia is home to ground-based observatories like the High Energy Spe…

astro-ph.HE2016★ 5 cited

Gamma-ray blazar spectra with H.E.S.S. II mono analysis: the case of PKS 2155-304 and PG 1553+113

D. Zaborov, A. M. Taylor, D. A. Sanchez +2

The addition of a 28 m Cherenkov telescope (CT5) to the H.E.S.S. array extended the experiment's sensitivity to lower energies, providing new opportunities for studies of Active Ga…

astro-ph.HE2016★ 38 cited

Gamma-ray blazar spectra with H.E.S.S. II mono analysis: the case of PKS 2155-304 and PG 1553+113

H. E. S. S. Collaboration, :, H. Abdalla +332

The addition of a 28 m Cherenkov telescope (CT5) to the H.E.S.S. array extended the experiment's sensitivity to lower energies. The lowest energy threshold is obtained using monosc…

astro-ph.HE2014★ 31 cited

Long-term monitoring of PKS 2155304 with ATOM and H.E.S.S.: investigation of optical/-ray correlations in different spectral states

A. Abramowski, F. Aharonian, F. Ait Benkhali +225

In this paper we report on the analysis of all the available optical and very high-energy -ray (200 GeV) data for the BL Lac object PKS 2155304, collected simultaneously w…