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Luigi Costamante

Researcher at Max Planck Society

Publications -  109
Citations -  14002

Luigi Costamante is an academic researcher from Max Planck Society. The author has contributed to research in topics: Blazar & High Energy Stereoscopic System. The author has an hindex of 56, co-authored 105 publications receiving 13434 citations. Previous affiliations of Luigi Costamante include Centre national de la recherche scientifique.

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Journal ArticleDOI

An Exceptional Very High Energy Gamma-Ray Flare of PKS 2155-304

Felix Aharonian, +125 more
TL;DR: In this paper, the average flux observed during an extreme gamma-ray outburst is I(>200 GeV) = (1.72$\pm$$0.05_{\rm stat}
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The Spectral Energy Distribution of Fermi bright blazars

A. A. Abdo, +109 more
TL;DR: In this article, the broad-band spectral properties of the gamma-ray selected blazars of the Fermi LAT Bright AGN Sample (LBAS) were investigated.
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Observations of the Crab nebula with HESS

Felix Aharonian, +106 more
TL;DR: In this paper, the Crab nebula was observed with the H.E.S. stereoscopic Cherenkov-telescope array between 2003 and 2005 for a total of 22.9 hours (after data quality selection).
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Energy Spectrum of Cosmic-Ray Electrons at TeV Energies

Felix Aharonian, +155 more
TL;DR: In this measurement, the first of this type, the High Energy Stereoscopic System is able to extend the measurement of the electron spectrum beyond the range accessible to direct measurements, finding evidence for a substantial steepening in the energy spectrum above 600 GeV compared to lower energies.
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A low level of extragalactic background light as revealed by gamma-rays from blazars.

Felix Aharonian, +102 more
- 20 Apr 2006 - 
TL;DR: In this paper, an alternative approach is proposed based on the detection and identification of EBL absorption features in high-energy spectra of objects of known redshift, which provides the most stringent upper limit to date on the EBL in the Opt-NIR band, which appears significantly lower than expected from the current direct estimates and very close to the absolute lower limit represented by the integrated light of resolved galaxies.