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N. Giglietto

Researcher at University of Bari

Publications -  224
Citations -  8263

N. Giglietto is an academic researcher from University of Bari. The author has contributed to research in topics: Cosmic ray & Fermi Gamma-ray Space Telescope. The author has an hindex of 43, co-authored 224 publications receiving 7623 citations.

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The Spectral Energy Distribution of Fermi bright blazars

A. A. Abdo, +109 more
TL;DR: In this article, the broad-band spectral properties of the gamma-ray selected blazars of the Fermi LAT Bright AGN Sample (LBAS) were investigated.
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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.
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Fermi LAT Search for Dark Matter in Gamma-Ray Lines and the Inclusive Photon Spectrum

Markus Ackermann, +119 more
- 05 Jul 2012 - 
TL;DR: In this article, the authors give cross section upper and decay lifetime lower limits for dark matter models that produce gamma-ray lines or contribute to the diffuse spectrum, including models proposed as explanations of the PAMELA and Fermi cosmic-ray data.
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Observations of Milky Way Dwarf Spheroidal galaxies with the Fermi-LAT detector and constraints on Dark Matter models

A. A. Abdo, +161 more
TL;DR: In this article, the gamma-ray flux of 14 dwarf spheroidal galaxies with the Fermi Gamma-Ray Space Telescope taken during the first 11 months of survey mode operations was determined, assuming both powerlaw spectra and representative spectra from WIMP annihilation.
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Measurement of the atmospheric neutrino-induced upgoing muon flux using MACRO

M. Ambrosio, +135 more
- 27 Aug 1998 - 
TL;DR: In this article, a measurement of the flux of neutrino-induced upgoing muons ( ν >∼ 100 GeV) using the MACRO detector is presented, where the ratio of the observed to expected events integrated over all zenith angles is 0.74 ± 0.036 (stat) ±0.13 (theoretical).