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F. Spada

Researcher at Istituto Nazionale di Fisica Nucleare

Publications -  63
Citations -  8094

F. Spada is an academic researcher from Istituto Nazionale di Fisica Nucleare. The author has contributed to research in topics: Fermi Gamma-ray Space Telescope & Cosmic ray. The author has an hindex of 37, co-authored 63 publications receiving 7276 citations.

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Searching for dark matter annihilation from Milky Way dwarf spheroidal galaxies with six years of Fermi Large Area Telescope data

Markus Ackermann, +125 more
TL;DR: In this article, the authors report on γ-ray observations of the Milky-Way satellite galaxies (dSphs) based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis.
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The Third Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope

Markus Ackermann, +183 more
TL;DR: The third catalog of active galactic nuclei (AGNs) detected by the Fermi-LAT (3LAC) is presented in this paper, which is based on the 3FGL of sources detected between 100 MeV and 300 GeV.
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The Third Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope

Markus Ackermann, +139 more
TL;DR: The third catalog of active galactic nuclei (AGNs) detected by the Fermi-LAT (3LAC) is presented in this article, which includes 1591 AGNs located at high Galactic latitudes (|b|>10°), a 71% increase over the second catalog based on 2 years of data.
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FERMI-LAT OBSERVATIONS of HIGH-ENERGY γ-RAY EMISSION TOWARD the GALACTIC CENTER

Marco Ajello, +158 more
TL;DR: The Fermi Large Area Telescope (LAT) has provided the most detailed view to date of the emission toward the Galactic center (GC) in high-energy gamma-rays as mentioned in this paper.
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Updated search for spectral lines from Galactic dark matter interactions with pass 8 data from the Fermi Large Area Telescope

Markus Ackermann, +119 more
- 29 May 2015 - 
TL;DR: In this article, the authors search for spectral lines in the Fermi Large Area Telescope observations of the Milky Way halo in the energy range 200 MeV-500 GeV using analysis methods from their most recent line searches.