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researcher

M. Holler

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

fields
  • astro-ph.HE3
same name
  • M. Holler — 9 papers
  • M. Holler — 8 papers, h 41
  • M. Holler — 1 paper, h 8

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedSearch for TeV Gamma-ray Emission from GRB 100621A, an extremely bright GRB in X-rays, with H.E.S.S

251 citations · 353 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2017★ 79 cited

Measurement of the EBL spectral energy distribution using the VHE gamma-ray spectra of H.E.S.S. blazars

H. E. S. S. Collaboration, :, H. Abdalla +256

Very high-energy gamma-rays (VHE, E>100 GeV) propagating over cosmological distances can interact with the low-energy photons of the extragalactic background light (EBL) and produc…

astro-ph.HE2014★ 251 cited

Search for TeV Gamma-ray Emission from GRB 100621A, an extremely bright GRB in X-rays, with H.E.S.S

H. E. S. S. Collaboration, A. Abramowski, F. Aharonian +213

The long gamma-ray burst (GRB) 100621A, at the time the brightest X-ray transient ever detected by Swift-XRT in the 0.3–10 keV range, has been observed with the H.E.S.S…

astro-ph.HE2014★ 23 cited

TeV γ-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S

H. E. S. S. Collaboration, A. Abramowski, F. Aharonian +217

The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 and G330.2+1.0 is an indication of intense particle acceleration in the shock fr…

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