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G

G. Pühlhofer

Researcher at University of Tübingen

Publications -  253
Citations -  12245

G. Pühlhofer is an academic researcher from University of Tübingen. The author has contributed to research in topics: Pulsar & Supernova remnant. The author has an hindex of 50, co-authored 247 publications receiving 10736 citations. Previous affiliations of G. Pühlhofer include Heidelberg University.

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Journal ArticleDOI

Letter of intent for KM3NeT 2.0

S. Adrián-Martínez, +246 more
- 24 Jun 2016 - 
TL;DR: In this article, the main objectives of the KM3NeT Collaboration are (i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and (ii) the determination of the mass hierarchy of neutrinos.
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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.
Journal ArticleDOI

Letter of Intent for KM3NeT 2.0

S. Adrián-Martínez, +245 more
TL;DR: In this paper, the main objectives of the KM3NeT Collaboration are the discovery and subsequent observation of high-energy neutrino sources in the Universe and the determination of the mass hierarchy of neutrinos.
Journal ArticleDOI

Discovery of very-high-energy |[gamma]|-rays from the Galactic Centre ridge

Felix Aharonian, +102 more
- 09 Feb 2006 - 
TL;DR: In this paper, a very high-energy γ-ray emission from the Galactic Centre region has been measured using HESS, the High Energy Stereoscopic System recently constructed in Namibia, South West Africa.
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Search for a Dark Matter annihilation signal from the Galactic Center halo with H.E.S.S

A. Abramowski, +193 more
TL;DR: Limits are derived on the velocity-weighted annihilation cross section (σv) as a function of the DM particle mass that are among the best reported so far for this energy range and in particular differ only little between the chosen density profile parametrizations.