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C. C. Hsu

Researcher at Max Planck Society

Publications -  56
Citations -  6268

C. C. Hsu is an academic researcher from Max Planck Society. The author has contributed to research in topics: Neutrino & Neutrino detector. The author has an hindex of 37, co-authored 54 publications receiving 5998 citations. Previous affiliations of C. C. Hsu include University of the Witwatersrand.

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Variable very high energy γ-ray emission from markarian 501

Justin Albert, +149 more
TL;DR: The MAGIC telescope was used to observe the blazar Markarian 501 (Mrk 501) at energies above 100 GeV from May through July 2005 as mentioned in this paper, and the high sensitivity of the instrument enabled the determination of the flux and spectrum of the source on a night-by-night basis.
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ANTARES: the first undersea neutrino telescope

M. Ageron, +287 more
TL;DR: The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational neutrino telescope in the Mediterranean Sea as mentioned in this paper, where the main purpose of the detector is to perform neutrinos astronomy and the apparatus also offers facilities for marine and Earth sciences.
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Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?

J. Albert, +148 more
- 27 Jun 2008 - 
TL;DR: The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detected very-high-energy gamma rays from a giant flare of the distant Quasi-Stellar Radio Source 3C 279, at a distance of more than 5 billion light-years.
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Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303.

Justin Albert, +148 more
- 23 Jun 2006 - 
TL;DR: The detection of variable gamma-ray emission above 100 gigaelectron volts from the microquasar LS I 61 + 303 is reported, which suggests that the emission is periodic.
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VHE γ-Ray Observation of the Crab Nebula and its Pulsar with the MAGIC Telescope

Justin Albert, +146 more
TL;DR: In this article, very high energy (VHE) gamma-ray observations of the Crab Nebula with the MAGIC telescope were reported, where the gamma spectrum can be described by a curved power law dF/dE = f(0)(E/300 GeV).