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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.

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A statistical approach to recognizing source classes for unassociated sources in the first Fermi-LAT catalog

Markus Ackermann, +215 more
TL;DR: In this article, the authors employed two statistical analyses of the primary gamma-ray characteristics for these unassociated sources in an effort to correlate their gamma ray properties with the AGN and pulsar populations in 1FGL.
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γ-RAY AND PARSEC-SCALE JET PROPERTIES OF A COMPLETE SAMPLE OF BLAZARS FROM THE MOJAVE PROGRAM

Matthew L. Lister, +174 more
TL;DR: In this paper, the Fermi LAT gamma-ray and 15 GHz VLBA radio properties of a joint Gamma-ray- and radio-selected sample of AGNs obtained during the first 11 months of the FERi mission (2008 Aug 4 - 2009 Jul 5) were investigated.
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The Search for Spatial Extension in High-latitude Sources Detected by the $Fermi$ Large Area Telescope

Markus Ackermann, +141 more
TL;DR: In this paper, a search for spatial extension in high-latitude sources in recent Fermi point source catalogs is presented, which provides source extensions and likelihood profiles for a suite of tested source morphologies.
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Impulsive and Long Duration High-Energy Gamma-ray Emission From the Very Bright 2012 March 7 Solar Flares

Marco Ajello, +163 more
TL;DR: In this paper, the Fermi Large Area Telescope (LAT) observed two bright X-class solar ares on 2012 March 7, and detected gamma-rays up to 4 GeV.
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PERIODIC VERY HIGH ENERGY γ-RAY EMISSION FROM LS I +61°303 OBSERVED WITH THE MAGIC TELESCOPE

Justin Albert, +153 more
TL;DR: In this paper, the MAGIC collaboration reported the discovery of γ-ray emission from the binary system LS I +61°303 in the TeV energy region, and the authors presented new observational results on this source in the energy range between 300 GeV and 3 TeV.