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Denis Bastieri

Researcher at University of Padua

Publications -  491
Citations -  67102

Denis Bastieri is an academic researcher from University of Padua. The author has contributed to research in topics: Fermi Gamma-ray Space Telescope & Blazar. The author has an hindex of 135, co-authored 473 publications receiving 62620 citations. Previous affiliations of Denis Bastieri include Istituto Nazionale di Fisica Nucleare & INAF.

Papers
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Magic gamma-ray telescope observation of the perseus cluster of galaxies : implications for cosmic rays, dark matter, and ngc 1275

Jelena Aleksić, +159 more
TL;DR: The MAGIC Cherenkov telescope was used to observe the Perseus galaxy cluster for a total effective time of 24.4 hours during 2008 November and December as discussed by the authors, and the resulting upper limits on the gamma-ray emission above 100 GeV are in the range of 4.6-7.5, thereby constraining the emission produced by cosmic rays, dark matter annihilations and the central radio galaxy NGC 1275.
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Fermi Observations of TeV-Selected Active Galactic Nuclei

A. A. Abdo, +225 more
TL;DR: In this article, the authors report on observations of TeV-selected active galactic nuclei (AGNs) made during the first 55 months of observations with the Large Area Telescope (LAT) on-board the Fermi Gamma-ray Space Telescope (Fermi).
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The 2010 very high energy gamma-ray flare & 10 years of multi-wavelength observations of M 87

A. Abramowski, +440 more
TL;DR: In this article, results from a joint very high energy (VHE; E>100 GeV) gamma-ray emission campaign on M 87 by the MAGIC and VERITAS instruments in 2010 are reported.
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Search for Dark Matter Satellites using the FERMI-LAT

Markus Ackermann, +134 more
TL;DR: In this article, the results of a large area telescope (LAT) search for dark matter satellites via the gamma-ray emission expected from the annihilation of weakly interacting massive particle (WIMP) dark matter were reported.
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Observations of the Large Magellanic Cloud with Fermi

A. A. Abdo, +217 more
TL;DR: In this paper, the distribution and sources of cosmic rays in the Large Magellanic Cloud (LMC) from analysis of gamma-ray observations were investigated and it was shown that cosmic rays are accelerated in massive star forming regions as a result of the large amounts of kinetic energy that are input by the stellar winds and supernova explosions of massive stars into the interstellar medium.